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aa class changes from Pit
git-svn-id: svn://svn.lyx.org/lyx/lyx-devel/trunk@2115 a592a061-630c-0410-9148-cb99ea01b6c8
This commit is contained in:
Jean-Marc Lasgouttes
parent
3e22b13963
commit
09316f3480
@ -1,3 +1,17 @@
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2001-06-12 Peter Suetterlin <P.Suetterlin@astro.uu.nl>
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* examples/aa_head.lyx:
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* examples/aa_paper.lyx: removed
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* doc/LaTeXConfig.lyx.in:
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* examples/aa_sample.lyx:
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* layouts/aa.layout:
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* layouts/aapaper.inc:
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* layouts/aapaper.layout:
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* templates/aa.lyx: aa.layout is for the new version of the
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A&A document class, while aapaper.layout is for the older (and
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slightly incompatible) version.
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2001-06-07 Jean-Marc Lasgouttes <Jean-Marc.Lasgouttes@inria.fr>
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* doc/LaTeXConfig.lyx.in:
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@ -24,12 +38,12 @@
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2001-05-22 Adrien Rebollo <rebollo@iaf.cnrs-gif.fr>
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* lib/kbd/european.kmap:
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* lib/kbd/francais.kmap:
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* lib/kbd/iso8859-15.cdef:
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* kbd/european.kmap:
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* kbd/francais.kmap:
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* kbd/iso8859-15.cdef:
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* encodings: add iso8859-15 support.
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* lib/kbd/iso8859-1.cdef: cleanup
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* kbd/iso8859-1.cdef: cleanup
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2001-05-22 Peter Suetterlin <P.Suetterlin@astro.uu.nl>
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@ -360,16 +360,16 @@ Additional document classes
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aa
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\layout Description
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Found: @chk_aapaper@
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Found: @chk_aa@
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\layout Description
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CTAN: N/A (available from Springer's ftp site
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CTAN: N/A (available from ftp site
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\family typewriter
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ftp.springer.de
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ftp.edpsciences.org
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\family default
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in directory
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\family typewriter
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/pub/tex/latex/aa
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/pub/aa/
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\family default
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)
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\layout Description
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@ -378,16 +378,13 @@ Notes: The document class
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\family sans
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aa
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\family default
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can be used to write articles for submission to the scientific journal
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(Version 5.01) can be used to write articles for submission to the
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scientific journal
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\emph on
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Astronomy and Astrophysics
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\emph default
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and the accompanying
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\emph on
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Supplement Series
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\emph default
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published by Springer -Verlag.
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published by EDP Sciences.
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\layout Subsection
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aastex
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@ -1,153 +0,0 @@
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#This file was created by <pit> Tue Nov 25 23:06:48 1997
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#LyX 0.11 (C) 1995-1997 Matthias Ettrich and the LyX Team
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\lyxformat 2.15
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\textclass aa
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\language english
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\inputencoding latin1
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\fontscheme times
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\graphics default
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\paperfontsize default
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\spacing single
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\papersize Default
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\paperpackage a4
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\use_geometry 0
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\use_amsmath 0
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\paperorientation portrait
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\secnumdepth 3
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\tocdepth 3
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\paragraph_separation indent
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\defskip medskip
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\quotes_language english
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\quotes_times 2
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\papercolumns 2
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\papersides 2
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\paperpagestyle default
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\layout Thesaurus
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Sorry, no thesaurus for that
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\layout Title
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The Use of LyX in Astronomy
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\layout Subtitle
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Looking towards a bright future
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\layout Author
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P.
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Sütterlin
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\latex latex
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\backslash
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inst{
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\latex default
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1
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\latex latex
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}
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\begin_float footnote
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\layout Standard
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\series medium
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\emph on
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Present Address:
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\emph default
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Universitäts-Sternwarte, Geismarlandstr.
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11, D-37083 Göttingen
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\end_float
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\latex latex
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\backslash
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and
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\latex default
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A.N.
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Coauthor
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\latex latex
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\backslash
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inst{
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\latex default
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2
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\latex latex
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}
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\layout Address
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Kiepenheuer-Institut für Sonnenphysik, Schöneckstr.
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6, D-79104 Freiburg
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\latex latex
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\backslash
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and
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\latex default
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Somewhere-in-the-Country
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\layout Offprint
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P.
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Sütterlin
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\layout Email
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pit@uni-sw.gwdg.de
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\layout Date
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Received: maybe / Accepted: who knows
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\layout Abstract
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In this paper we show that LyX can be used to write papers for puplication
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in the journal Astronomy and Astrophysics.
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\layout Abstract
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\latex latex
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\backslash
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keywords{
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\latex default
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LaTeX - Wordprocessing - Publication
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\latex latex
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}
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\layout Section
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Intoduction
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\layout Standard
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In 1997, Springer Verlag decided to accept papers for publication in their
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journals
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\emph on
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Astronomy and Astrophysics
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\emph default
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and the acompanying
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\emph on
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Supplement Series
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\emph default
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only in form of LaTeX.
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At the same time, they switched the layout macros to LaTeX2
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\begin_inset Formula \( \epsilon \)
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\end_inset
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(Lamport
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\begin_inset LatexCommand \cite{kopka}
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\end_inset
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).
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This made it easy to adapt a corresponding LyX style to produce the correct
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output for direct submission to A&A.
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\layout Section
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Discussion
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\layout Standard
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What is there to discuss about? The existence of LyX with this layout makes
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it as easy as one could wish to write scientific papers.
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\layout Bibliography
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\bibitem [1994]{lamport}
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L.
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Lamport, 1994:
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\emph on
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LaTeX: A Document Preparation System
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\emph default
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, Addison-Wesley Publishing Company, 2nd edition
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\the_end
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@ -1,8 +1,12 @@
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#LyX 1.1 created this file. For more info see http://www.lyx.org/
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\lyxformat 218
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\textclass aa
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\begin_preamble
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\usepackage{graphicx}
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%
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\end_preamble
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\language english
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\inputencoding latin1
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\inputencoding auto
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\fontscheme default
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\graphics default
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\paperfontsize default
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@ -22,9 +26,6 @@
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\papersides 2
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\paperpagestyle default
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\layout Thesaurus
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06(03.11.1;16.06.1;19.06.1;19.37.1;19.53.1;19.63.1)
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\layout Title
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Hydrodynamics of giant planet formation
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@ -39,21 +40,68 @@ I.
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\layout Author
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G.
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Wuchterl
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\layout Address
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Wuchterl
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\latex latex
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Institute for Astronomy (IfA), University of Vienna, Türkenschanzstrasse
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17, A-1180 Vienna
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\backslash
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inst{1}
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\backslash
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and
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\newline
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\latex default
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C.
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Ptolemy
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\latex latex
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\backslash
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inst{2}
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\backslash
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fnmsep
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\begin_float footnote
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\layout Standard
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Just to show the usage of the elements in the author field
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\end_float
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\layout Offprint
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G.
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Wuchterl
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\layout Email
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\layout Address
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wuchterl@amok.ast.univie.ac.at
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Institute for Astronomy (IfA), University of Vienna, T\i \"{u}
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rkenschanzstrasse
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17, A-1180 Vienna
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\newline
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\latex latex
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\backslash
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email{wuchterl@amok.ast.univie.ac.at}
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\backslash
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and
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\newline
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\latex default
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University of Alexandria, Department of Geography, ...
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\newline
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\latex latex
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\backslash
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email{c.ptolemy@hipparch.uheaven.space}
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\latex default
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\begin_float footnote
|
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\layout Standard
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The university of heaven temporarily does not accept e-mails
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\end_float
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\layout Date
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Received September 15, 1996 / Accepted March 16, 1997
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Received September 15, 1996; accepted March 16, 1997
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\layout Abstract
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To investigate the physical nature of the `nuc\SpecialChar \-
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@ -74,9 +122,7 @@ leated instability' of proto
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opacities and the local thermodynamic state in the layer.
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Stability and instability can therefore be expressed in the form of stability
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equations of state which are universal for a given composition.
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\layout Abstract
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||||
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The stability equations of state are calculated for solar composition and
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The stability equations of state are calculated for solar composition and
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are displayed in the domain
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\begin_inset Formula \( -14\leq \lg \rho /[\mathrm{g}\, \mathrm{cm}^{-3}]\leq 0 \)
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\end_inset
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@ -103,7 +149,7 @@ The stability equations of state are calculated for solar composition and
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.
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Regions of instability in the
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\begin_inset Formula \( (\rho \, e) \)
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\begin_inset Formula \( (\rho ,e) \)
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\end_inset
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-plane are described and related to the underlying microphysical processes.
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@ -114,21 +160,20 @@ The stability equations of state are calculated for solar composition and
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\end_inset
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-mechanism is widespread under `cool' conditions.
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\layout Abstract
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\latex latex
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\newline
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\backslash
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keywords{
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keywords{giant planet formation --
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\backslash
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(
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\backslash
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kappa
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\backslash
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)-mechanism -- stability of gas spheres }
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\latex default
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giant planet formation --
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\begin_inset Formula \( \kappa \)
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\end_inset
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-mechanism -- stability of gas spheres
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\latex latex
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}
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\layout Section
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Introduction
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@ -137,7 +182,12 @@ Introduction
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In the
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\emph on
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nucleated instability
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\latex latex
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\backslash
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/{}
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\emph default
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\latex default
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(also called core instability) hypothesis of giant planet formation, a
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critical mass for static core envelope protoplanets has been found.
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Mizuno (
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@ -171,37 +221,12 @@ Although no hydrodynamical study has been available many workers conjectured
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\end_inset
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) standard one-zone model.
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The nonlinear, hydrodynamic evolution of the protogiant planet beyond the
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critical mass, as calculated by Wuchterl (
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\begin_inset LatexCommand \cite{wuchterl}
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\end_inset
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), will be described in a forthcoming article.
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\layout Standard
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The fact that Wuchterl (
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\begin_inset LatexCommand \cite{wuchterl}
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\end_inset
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) found the excitation of hydrodynamical waves in his models raises considerable
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interest on the transition from static to dynamic evolutionary phases of
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the protogiant planet at the critical mass.
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The waves play a crucial role in the development of the so-called nucleated
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instability in the nucleated instability hypothesis.
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They lead to the formation of shock waves and massive outflow phenomena.
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The protoplanet evolves into a new quasi-equilibrium structure with a
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\emph on
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pulsating
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\emph default
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envelope, after the mass loss phase has declined.
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\layout Standard
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Phenomena similar to the ones described above for giant planet formation
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have been found in hydrodynamical models concerning star formation where
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protostellar cores explode (Tscharnuter
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\begin_inset LatexCommand \cite{tscarnuter}
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\begin_inset LatexCommand \cite{tscharnuter}
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\end_inset
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@ -220,21 +245,10 @@ Baker's standard one-zone model
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\layout Standard
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\begin_float wide-fig
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\layout Standard
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\latex latex
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\backslash
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rule{0.4pt}{4cm}
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\hfill
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\backslash
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parbox[b]{55mm}{
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\layout Caption
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Adiabatic exponent
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\begin_inset Formula \( \Gamma \)
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\begin_inset Formula \( \Gamma _{1} \)
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\end_inset
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.
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@ -242,7 +256,7 @@ Adiabatic exponent
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\begin_inset Formula \( \Gamma _{1} \)
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\end_inset
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is plotted as a function of
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is plotted as a function of
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\begin_inset Formula \( \lg \)
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\end_inset
|
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@ -259,20 +273,22 @@ is plotted as a function of
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\end_inset
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\layout Standard
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\begin_inset LatexCommand \label{FigGam}
|
||||
|
||||
\end_inset
|
||||
|
||||
|
||||
\latex latex
|
||||
}
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||||
\end_float
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||||
In this section the one-zone model of Baker (
|
||||
In this section the one-zone model of Baker (
|
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\begin_inset LatexCommand \cite{baker}
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||||
|
||||
\end_inset
|
||||
|
||||
), originally used to study the Cepheïd pulsation mechanism, will be briefly
|
||||
), originally used to study the Cephe\i \"{\i}
|
||||
d pulsation mechanism, will be briefly
|
||||
reviewed.
|
||||
The resulting stability criteria will be rewritten in terms of local state
|
||||
variables, local timescales and constitutive relations.
|
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@ -284,20 +300,26 @@ Baker (
|
||||
\end_inset
|
||||
|
||||
) investigates the stability of thin layers in self-gravitating, spherical
|
||||
gas clouds with the following properties:
|
||||
gas clouds with the following properties:
|
||||
\layout Itemize
|
||||
|
||||
hydrostatic equilibrium,
|
||||
hydrostatic equilibrium,
|
||||
\layout Itemize
|
||||
|
||||
thermal equilibrium,
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||||
thermal equilibrium,
|
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\layout Itemize
|
||||
|
||||
energy transport by grey radiation diffusion.
|
||||
|
||||
\layout Standard
|
||||
|
||||
\noindent
|
||||
For the one-zone-model Baker obtains necessary conditions for dynamical,
|
||||
secular and vibrational (or pulsational) stability [Eqs.\SpecialChar ~
|
||||
secular and vibrational (or pulsational) stability (Eqs.
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
|
||||
\latex default
|
||||
(34a,
|
||||
\latex latex
|
||||
|
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@ -315,53 +337,60 @@ c) in Baker
|
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\end_inset
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||||
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].
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).
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||||
Using Baker's notation:
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\layout Standard
|
||||
\align left
|
||||
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||||
\begin_inset Formula \begin{eqnarray*}
|
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M_{\mathrm{r}} & & \mathrm{mass}\, \mathrm{internal}\, \mathrm{to}\, \mathrm{the}\, \mathrm{radius}\, r\\
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m & & \mathrm{mass}\, \mathrm{of}\, \mathrm{the}\, \mathrm{zone}\\
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r_{0} & & \mathrm{unperturbed}\, \mathrm{zone}\, \mathrm{radius}\\
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\rho _{0} & & \mathrm{unperturbed}\, \mathrm{density}\, \mathrm{in}\, \mathrm{the}\, \mathrm{zone}\\
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T_{0} & & \mathrm{unperturbed}\, \mathrm{temperature}\, \mathrm{in}\, \mathrm{the}\, \mathrm{zone}\\
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L_{r0} & & \mathrm{unperturbed}\, \mathrm{luminosity}\\
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E_{\mathrm{th}} & & \mathrm{thermal}\, \mathrm{energy}\, \mathrm{of}\, \mathrm{the}\, \mathrm{zone}
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M_{r} & & \textrm{mass internal to the radius }r\\
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||||
m & & \textrm{mass of the zone}\\
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||||
r_{0} & & \textrm{unperturbed zone radius}\\
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||||
\rho _{0} & & \textrm{unperturbed density in the zone}\\
|
||||
T_{0} & & \textrm{unperturbed temperature in the zone}\\
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||||
L_{r0} & & \textrm{unperturbed luminosity}\\
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||||
E_{\textrm{th}} & & \textrm{thermal energy of the zone}
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\end{eqnarray*}
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\end_inset
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||||
|
||||
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\layout Standard
|
||||
\noindent
|
||||
and with the definitions of the
|
||||
\emph on
|
||||
local cooling time
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
/{}
|
||||
\emph default
|
||||
\latex default
|
||||
(see Fig.\SpecialChar ~
|
||||
|
||||
\begin_inset LatexCommand \ref{FigGam}
|
||||
|
||||
\end_inset
|
||||
|
||||
)
|
||||
\layout Standard
|
||||
|
||||
|
||||
)
|
||||
\begin_inset Formula \begin{equation}
|
||||
\tau _{\mathrm{co}}=\frac{E_{\mathrm{th}}}{L_{r0}}\, ,
|
||||
\end{equation}
|
||||
|
||||
\end_inset
|
||||
|
||||
and the
|
||||
and the
|
||||
\emph on
|
||||
local free-fall time
|
||||
\layout Standard
|
||||
|
||||
\emph default
|
||||
|
||||
\begin_inset Formula \begin{equation}
|
||||
\tau _{\mathrm{ff}}=\sqrt{\frac{3\pi }{32G}\frac{4\pi r_{0}^{3}}{3M_{\mathrm{r}}}\, ,}
|
||||
\tau _{\mathrm{ff}}=\sqrt{\frac{3\pi }{32G}\frac{4\pi r_{0}^{3}}{3M_{\mathrm{r}}}}\, ,
|
||||
\end{equation}
|
||||
|
||||
\end_inset
|
||||
|
||||
Baker's
|
||||
Baker's
|
||||
\begin_inset Formula \( K \)
|
||||
\end_inset
|
||||
|
||||
@ -369,7 +398,7 @@ Baker's
|
||||
\begin_inset Formula \( \sigma _{0} \)
|
||||
\end_inset
|
||||
|
||||
have the following form:
|
||||
have the following form:
|
||||
\begin_inset Formula \begin{eqnarray}
|
||||
\sigma _{0} & = & \frac{\pi }{\sqrt{8}}\frac{1}{\tau _{\mathrm{ff}}}\\
|
||||
K & = & \frac{\sqrt{32}}{\pi }\frac{1}{\delta }\frac{\tau _{\mathrm{ff}}}{\tau _{\mathrm{co}}}\, ;
|
||||
@ -377,14 +406,11 @@ K & = & \frac{\sqrt{32}}{\pi }\frac{1}{\delta }\frac{\tau _{\mathrm{ff}}}{\tau _
|
||||
|
||||
\end_inset
|
||||
|
||||
where
|
||||
\begin_inset Formula \( E_{\mathrm{th}}\approx m(P_{0}/\rho _{0}) \)
|
||||
where
|
||||
\begin_inset Formula \( E_{\mathrm{th}}\approx m(P_{0}/{\rho _{0}}) \)
|
||||
\end_inset
|
||||
|
||||
has been used and
|
||||
\layout Standard
|
||||
|
||||
|
||||
has been used and
|
||||
\begin_inset Formula \begin{equation}
|
||||
\begin{array}{l}
|
||||
\delta =-\left( \frac{\partial \ln \rho }{\partial \ln T}\right) _{P}\\
|
||||
@ -394,7 +420,7 @@ e=mc^{2}
|
||||
|
||||
\end_inset
|
||||
|
||||
is a thermodynamical quantity which is of order
|
||||
is a thermodynamical quantity which is of order
|
||||
\begin_inset Formula \( 1 \)
|
||||
\end_inset
|
||||
|
||||
@ -425,36 +451,35 @@ is a thermodynamical quantity which is of order
|
||||
Substituting into Baker's criteria, using thermodynamic identities and
|
||||
definitions of thermodynamic quantities,
|
||||
\begin_inset Formula \[
|
||||
\Gamma _{1}=\left( \frac{\partial \ln P}{\partial \ln \rho }\right) _{S}\, ,\: \chi _{\rho }=\left( \frac{\partial \ln P}{\partial \ln \rho }\right) _{T}\, ,\: \kappa _{P}=\left( \frac{\partial \ln \kappa }{\partial \ln P}\right) _{T}\]
|
||||
\Gamma _{1}=\left( \frac{\partial \ln P}{\partial \ln \rho }\right) _{S}\, ,\; \chi ^{}_{\rho }=\left( \frac{\partial \ln P}{\partial \ln \rho }\right) _{T}\, ,\; \kappa ^{}_{P}=\left( \frac{\partial \ln \kappa }{\partial \ln P}\right) _{T}\]
|
||||
|
||||
\end_inset
|
||||
|
||||
|
||||
\layout Standard
|
||||
|
||||
|
||||
\begin_inset Formula \[
|
||||
\nabla _{\mathrm{ad}}=\left( \frac{\partial \ln T}{\partial \ln P}\right) _{S}\, ,\: \chi _{T}=\left( \frac{\partial \ln P}{\partial \ln T}\right) _{\rho }\, ,\: \kappa _{T}=\left( \frac{\partial \ln \kappa }{\partial \ln P}\right) _{T}\]
|
||||
\nabla _{\mathrm{ad}}=\left( \frac{\partial \ln T}{\partial \ln P}\right) _{S}\, ,\; \chi ^{}_{T}=\left( \frac{\partial \ln P}{\partial \ln T}\right) _{\rho }\, ,\; \kappa ^{}_{T}=\left( \frac{\partial \ln \kappa }{\partial \ln T}\right) _{T}\]
|
||||
|
||||
\end_inset
|
||||
|
||||
one obtains, after some pages of algebra, the conditions for
|
||||
one obtains, after some pages of algebra, the conditions for
|
||||
\emph on
|
||||
stability
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
/{}
|
||||
\emph default
|
||||
given below:
|
||||
\layout Standard
|
||||
|
||||
|
||||
\latex default
|
||||
given below:
|
||||
\begin_inset Formula \begin{eqnarray}
|
||||
\frac{\pi ^{2}}{8}\frac{1}{\tau _{\mathrm{ff}}^{2}}(3\Gamma _{1}-4) & > & 0\label{ZSDynSta} \\
|
||||
\frac{\pi ^{2}}{\tau _{\mathrm{co}}\tau _{\mathrm{ff}}^{2}}\Gamma _{1}\nabla _{\mathrm{ad}}\left[ \frac{1-3/4\chi _{\rho }}{\chi _{T}}(\kappa _{T}-4)+\kappa _{P}+1\right] & > & 0\label{ZSSecSta} \\
|
||||
\frac{\pi ^{2}}{4}\frac{3}{\tau _{\mathrm{co}}\tau _{\mathrm{ff}}^{2}}\Gamma _{1}^{2}\nabla _{\mathrm{ad}}\left[ 4\nabla _{\mathrm{ad}}-(\nabla _{\mathrm{ad}}\kappa _{T}+\kappa _{P})-\frac{4}{3\Gamma _{1}}\right] & > & 0\label{ZSVibSta}
|
||||
\frac{\pi ^{2}}{\tau _{\mathrm{co}}\tau _{\mathrm{ff}}^{2}}\Gamma _{1}\nabla _{\mathrm{ad}}\left[ \frac{1-3/4\chi ^{}_{\rho }}{\chi ^{}_{T}}(\kappa ^{}_{T}-4)+\kappa ^{}_{P}+1\right] & > & 0\label{ZSSecSta} \\
|
||||
\frac{\pi ^{2}}{4}\frac{3}{\tau _{\mathrm{co}}\tau _{\mathrm{ff}}^{2}}\Gamma _{1}^{2}\, \nabla _{\mathrm{ad}}\left[ 4\nabla _{\mathrm{ad}}-(\nabla _{\mathrm{ad}}\kappa ^{}_{T}+\kappa ^{}_{P})-\frac{4}{3\Gamma _{1}}\right] & > & 0\label{ZSVibSta}
|
||||
\end{eqnarray}
|
||||
|
||||
\end_inset
|
||||
|
||||
For a physical discussion of the stability criteria see Baker (
|
||||
For a physical discussion of the stability criteria see Baker (
|
||||
\begin_inset LatexCommand \cite{baker}
|
||||
|
||||
\end_inset
|
||||
@ -468,13 +493,14 @@ For a physical discussion of the stability criteria see Baker (
|
||||
\layout Standard
|
||||
|
||||
We observe that these criteria for dynamical, secular and vibrational stability,
|
||||
respectively, can be factorized into
|
||||
respectively, can be factorized into
|
||||
\layout Enumerate
|
||||
|
||||
a factor containing local timescales only,
|
||||
a factor containing local timescales only,
|
||||
\layout Enumerate
|
||||
|
||||
a factor containing only constitutive relations and their derivatives.
|
||||
|
||||
\layout Standard
|
||||
|
||||
The first factors, depending on only timescales, are positive by definition.
|
||||
@ -499,13 +525,18 @@ The first factors, depending on only timescales, are positive by definition.
|
||||
Since they depend only on state variables, the stability criteria themselves
|
||||
are
|
||||
\emph on
|
||||
functions of the thermodynamic state in the local zone
|
||||
functions of the thermodynamic state in the local zone
|
||||
\emph default
|
||||
.
|
||||
The one-zone stability can therefore be determined from a simple equation
|
||||
of state, given for example, as a function of density and temperature.
|
||||
Once the microphysics, i.e.
|
||||
the thermodynamics and opacities (see Table\SpecialChar ~
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
|
||||
\latex default
|
||||
the thermodynamics and opacities (see Table\SpecialChar ~
|
||||
|
||||
\begin_inset LatexCommand \ref{KapSou}
|
||||
|
||||
@ -523,12 +554,12 @@ functions of the thermodynamic state in the local zone
|
||||
\begin_float tab
|
||||
\layout Caption
|
||||
|
||||
Opacity sources
|
||||
|
||||
\begin_inset LatexCommand \label{KapSou}
|
||||
|
||||
\end_inset
|
||||
|
||||
|
||||
Opacity sources
|
||||
\layout Standard
|
||||
|
||||
|
||||
@ -537,7 +568,7 @@ Opacity sources
|
||||
<features rotate="false" islongtable="false" endhead="0" endfirsthead="0" endfoot="0" endlastfoot="0">
|
||||
<column alignment="left" valignment="top" leftline="false" rightline="false" width="" special="">
|
||||
<column alignment="left" valignment="top" leftline="false" rightline="false" width="" special="">
|
||||
<row topline="true" bottomline="true" newpage="false">
|
||||
<row topline="true" bottomline="false" newpage="false">
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="false" rotate="false" usebox="none" width="" special="">
|
||||
\begin_inset Text
|
||||
|
||||
@ -546,16 +577,20 @@ Opacity sources
|
||||
Source
|
||||
\end_inset
|
||||
</cell>
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="true" rotate="false" usebox="none" width="" special="">
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="false" rotate="false" usebox="none" width="" special="">
|
||||
\begin_inset Text
|
||||
|
||||
\layout Standard
|
||||
|
||||
T/[K]
|
||||
|
||||
\begin_inset Formula \( T/[\textrm{K}] \)
|
||||
\end_inset
|
||||
|
||||
|
||||
\end_inset
|
||||
</cell>
|
||||
</row>
|
||||
<row topline="false" bottomline="false" newpage="false">
|
||||
<row topline="true" bottomline="false" newpage="false">
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="false" rotate="false" usebox="none" width="" special="">
|
||||
\begin_inset Text
|
||||
|
||||
@ -564,13 +599,13 @@ T/[K]
|
||||
Yorke 1979, Yorke 1980a
|
||||
\end_inset
|
||||
</cell>
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="true" rotate="false" usebox="none" width="" special="">
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="false" rotate="false" usebox="none" width="" special="">
|
||||
\begin_inset Text
|
||||
|
||||
\layout Standard
|
||||
|
||||
|
||||
\begin_inset Formula \( \leq 1700^{\mathrm{a}} \)
|
||||
\begin_inset Formula \( \leq 1700^{\textrm{a}} \)
|
||||
\end_inset
|
||||
|
||||
|
||||
@ -586,7 +621,7 @@ Yorke 1979, Yorke 1980a
|
||||
Krügel 1971
|
||||
\end_inset
|
||||
</cell>
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="true" rotate="false" usebox="none" width="" special="">
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="false" rotate="false" usebox="none" width="" special="">
|
||||
\begin_inset Text
|
||||
|
||||
\layout Standard
|
||||
@ -608,7 +643,7 @@ Kr
|
||||
Cox & Stewart 1969
|
||||
\end_inset
|
||||
</cell>
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="true" rotate="false" usebox="none" width="" special="">
|
||||
<cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="false" rotate="false" usebox="none" width="" special="">
|
||||
\begin_inset Text
|
||||
|
||||
\layout Standard
|
||||
@ -617,7 +652,7 @@ Cox & Stewart 1969
|
||||
\begin_inset Formula \( 5000\leq \)
|
||||
\end_inset
|
||||
|
||||
|
||||
|
||||
\end_inset
|
||||
</cell>
|
||||
</row>
|
||||
@ -627,31 +662,14 @@ Cox & Stewart 1969
|
||||
|
||||
|
||||
\layout Standard
|
||||
\added_space_top medskip*
|
||||
|
||||
|
||||
\begin_inset Formula \( ^{\textrm{a}} \)
|
||||
\end_inset
|
||||
|
||||
This is footnote a
|
||||
This is footnote a
|
||||
\end_float
|
||||
\begin_float wide-tab
|
||||
\layout Caption
|
||||
|
||||
Regions of secular instability
|
||||
\begin_inset LatexCommand \label{TabSecInst}
|
||||
|
||||
\end_inset
|
||||
|
||||
|
||||
\layout Standard
|
||||
|
||||
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
vspace{4cm}
|
||||
\end_float
|
||||
We will now write down the sign (and therefore stability) determining parts
|
||||
We will now write down the sign (and therefore stability) determining parts
|
||||
of the left-hand sides of the inequalities (
|
||||
\begin_inset LatexCommand \ref{ZSDynSta}
|
||||
|
||||
@ -684,47 +702,38 @@ The sign determining part of inequality\SpecialChar ~
|
||||
\begin_inset Formula \( 3\Gamma _{1}-4 \)
|
||||
\end_inset
|
||||
|
||||
and it reduces to the criterion for dynamical stability
|
||||
\layout Standard
|
||||
|
||||
|
||||
and it reduces to the criterion for dynamical stability
|
||||
\begin_inset Formula \begin{equation}
|
||||
\Gamma _{1}>\frac{4}{3}
|
||||
\Gamma _{1}>\frac{4}{3}\, \cdot
|
||||
\end{equation}
|
||||
|
||||
\end_inset
|
||||
|
||||
Stability of the thermodynamical equilibrium demands
|
||||
Stability of the thermodynamical equilibrium demands
|
||||
\begin_inset Formula \begin{equation}
|
||||
\chi _{\rho }>0,\: \: c_{v}>0\, ,
|
||||
\chi ^{}_{\rho }>0,\; \; c_{v}>0\, ,
|
||||
\end{equation}
|
||||
|
||||
\end_inset
|
||||
|
||||
and
|
||||
\layout Standard
|
||||
|
||||
|
||||
and
|
||||
\begin_inset Formula \begin{equation}
|
||||
\chi _{T}>0
|
||||
\chi ^{}_{T}>0
|
||||
\end{equation}
|
||||
|
||||
\end_inset
|
||||
|
||||
holds for a wide range of physical situations.
|
||||
With
|
||||
\layout Standard
|
||||
|
||||
|
||||
holds for a wide range of physical situations.
|
||||
With
|
||||
\begin_inset Formula \begin{eqnarray}
|
||||
\Gamma _{3}-1=\frac{P}{\rho T}\frac{\chi _{T}}{c_{v}} & > & 0\\
|
||||
\Gamma _{1}=\chi _{\rho }+\chi _{T}(\Gamma _{3}-1) & > & 0\\
|
||||
\Gamma _{3}-1=\frac{P}{\rho T}\frac{\chi ^{}_{T}}{c_{v}} & > & 0\\
|
||||
\Gamma _{1}=\chi _{\rho }^{}+\chi _{T}^{}(\Gamma _{3}-1) & > & 0\\
|
||||
\nabla _{\mathrm{ad}}=\frac{\Gamma _{3}-1}{\Gamma _{1}} & > & 0
|
||||
\end{eqnarray}
|
||||
|
||||
\end_inset
|
||||
|
||||
we find the sign determining terms in inequalities\SpecialChar ~
|
||||
we find the sign determining terms in inequalities\SpecialChar ~
|
||||
(
|
||||
\begin_inset LatexCommand \ref{ZSSecSta}
|
||||
|
||||
@ -740,20 +749,17 @@ we find the sign determining terms in inequalities\SpecialChar ~
|
||||
\emph on
|
||||
stability
|
||||
\emph default
|
||||
, respectively:
|
||||
\layout Standard
|
||||
|
||||
|
||||
, respectively:
|
||||
\begin_inset Formula \begin{eqnarray}
|
||||
3\Gamma _{1}-4=:\, S_{\mathrm{dyn}}> & 0 & \label{DynSta} \\
|
||||
\frac{1-3/4\chi _{\rho }}{\chi _{T}}(\kappa _{T}-4)+\kappa _{P}+1=:\, S_{\mathrm{sec}}> & 0 & \label{SecSta} \\
|
||||
4\nabla _{\mathrm{ad}}-(\nabla _{\mathrm{ad}}\kappa _{T}+\kappa _{P}-\frac{4}{3\Gamma _{1}}=:\, S_{\mathrm{vib}}> & 0 & \label{VibSta}
|
||||
3\Gamma _{1}-4=:S_{\mathrm{dyn}}> & 0 & \label{DynSta} \\
|
||||
\frac{1-3/4\chi ^{}_{\rho }}{\chi ^{}_{T}}(\kappa ^{}_{T}-4)+\kappa ^{}_{P}+1=:S_{\mathrm{sec}}> & 0 & \label{SecSta} \\
|
||||
4\nabla _{\mathrm{ad}}-(\nabla _{\mathrm{ad}}\kappa ^{}_{T}+\kappa ^{}_{P})-\frac{4}{3\Gamma _{1}}=:S_{\mathrm{vib}}> & 0\, . & \label{VibSta}
|
||||
\end{eqnarray}
|
||||
|
||||
\end_inset
|
||||
|
||||
The constitutive relations are to be evaluated for the unperturbed thermodynamic
|
||||
state (say
|
||||
The constitutive relations are to be evaluated for the unperturbed thermodynami
|
||||
c state (say
|
||||
\begin_inset Formula \( (\rho _{0},T_{0}) \)
|
||||
\end_inset
|
||||
|
||||
@ -768,11 +774,11 @@ e relations
|
||||
\end_inset
|
||||
|
||||
,
|
||||
\begin_inset Formula \( \chi _{T},\, \chi _{\rho } \)
|
||||
\begin_inset Formula \( \chi _{T}^{},\, \chi _{\rho }^{} \)
|
||||
\end_inset
|
||||
|
||||
,
|
||||
\begin_inset Formula \( \kappa _{P},\, \kappa _{T} \)
|
||||
\begin_inset Formula \( \kappa _{P}^{},\, \kappa _{T}^{} \)
|
||||
\end_inset
|
||||
|
||||
.
|
||||
@ -799,22 +805,10 @@ e relations
|
||||
|
||||
.
|
||||
Regions of secular instability are listed in Table\SpecialChar ~
|
||||
|
||||
\begin_inset LatexCommand \ref{TabSecInst}
|
||||
|
||||
\end_inset
|
||||
|
||||
.
|
||||
1.
|
||||
\layout Standard
|
||||
|
||||
\begin_float fig
|
||||
\layout Standard
|
||||
|
||||
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
vspace{5cm}
|
||||
\layout Caption
|
||||
|
||||
Vibrational stability equation of state
|
||||
@ -826,7 +820,10 @@ Vibrational stability equation of state
|
||||
\begin_inset Formula \( >0 \)
|
||||
\end_inset
|
||||
|
||||
means vibrational stability.
|
||||
means vibrational stability
|
||||
\layout Standard
|
||||
|
||||
|
||||
\begin_inset LatexCommand \label{FigVibStab}
|
||||
|
||||
\end_inset
|
||||
@ -847,11 +844,13 @@ The conditions for the stability of static, radiative layers in gas spheres,
|
||||
) standard one-zone model, can be expressed as stability equations of state.
|
||||
These stability equations of state depend only on the local thermodynamic
|
||||
state of the layer.
|
||||
|
||||
\layout Enumerate
|
||||
|
||||
If the constitutive relations -- equations of state and Rosseland mean opacities
|
||||
-- are specified, the stability equations of state can be evaluated without
|
||||
specifying properties of the layer.
|
||||
|
||||
\layout Enumerate
|
||||
|
||||
For solar composition gas the
|
||||
@ -866,7 +865,9 @@ For solar composition gas the
|
||||
dissociation and the combined H, first He ionization zone, as indicated
|
||||
by vibrational instability.
|
||||
These regions of instability are much larger in extent and degree of instabilit
|
||||
y than the second He ionization zone that drives the Cepheïd pulsations.
|
||||
y than the second He ionization zone that drives the Cephe\i \"{\i}
|
||||
d pulsations.
|
||||
|
||||
\layout Acknowledgement
|
||||
|
||||
Part of this work was supported by the German
|
||||
@ -877,81 +878,86 @@ schungs\SpecialChar \-
|
||||
ge\SpecialChar \-
|
||||
mein\SpecialChar \-
|
||||
schaft, DFG
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
/{}
|
||||
\emph default
|
||||
\latex default
|
||||
project number Ts\SpecialChar ~
|
||||
17/2--1.
|
||||
|
||||
\layout Bibliography
|
||||
\bibitem [1966]{baker}
|
||||
|
||||
Baker N., 1966, in: Stellar Evolution, eds.\SpecialChar ~
|
||||
Baker, N.
|
||||
1966, in Stellar Evolution, ed.
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
|
||||
\latex default
|
||||
R.
|
||||
F.
|
||||
Stein, A.
|
||||
Stein,& A.
|
||||
G.
|
||||
W.
|
||||
Cameron, Plenum, New York, p.\SpecialChar ~
|
||||
333
|
||||
Cameron (Plenum, New York) 333
|
||||
\layout Bibliography
|
||||
\bibitem [1988]{balluch}
|
||||
|
||||
Balluch M., 1988, A&A 200, 58
|
||||
Balluch, M.
|
||||
1988, A&A, 200, 58
|
||||
\layout Bibliography
|
||||
\bibitem [1980]{cox}
|
||||
|
||||
Cox J.
|
||||
P., 1980, Theory of Stellar Pulsation, Princeton University Press, Princeton,
|
||||
p.\SpecialChar ~
|
||||
165
|
||||
Cox, J.
|
||||
P.
|
||||
1980, Theory of Stellar Pulsation (Princeton University Press, Princeton)
|
||||
165
|
||||
\layout Bibliography
|
||||
\bibitem [1969]{cox69}
|
||||
|
||||
Cox A.
|
||||
N., Stewart J.
|
||||
N., 1969, Academia Nauk, Scientific Information 15, 1
|
||||
\layout Bibliography
|
||||
\bibitem [1971]{kruegel}
|
||||
|
||||
Krügel E., 1971, Der Rosselandsche Mittelwert bei tiefen Temperaturen, Diplom--Th
|
||||
esis, Univ.\SpecialChar ~
|
||||
Göttingen
|
||||
Cox, A.
|
||||
N.,& Stewart, J.
|
||||
N.
|
||||
1969, Academia Nauk, Scientific Information 15, 1
|
||||
\layout Bibliography
|
||||
\bibitem [1980]{mizuno}
|
||||
|
||||
Mizuno H., 1980, Prog.
|
||||
Mizuno H.
|
||||
1980, Prog.
|
||||
Theor.
|
||||
Phys.
|
||||
64, 544
|
||||
Phys., 64, 544
|
||||
\layout Bibliography
|
||||
\bibitem [1987]{tscarnuter}
|
||||
\bibitem [1987]{tscharnuter}
|
||||
|
||||
Tscharnuter W.
|
||||
M., 1987, A&A 188, 55
|
||||
Tscharnuter W.
|
||||
M.
|
||||
1987, A&A, 188, 55
|
||||
\layout Bibliography
|
||||
\bibitem [1989]{wuchterl}
|
||||
\bibitem [1992]{terlevich}
|
||||
|
||||
Wuchterl G., 1989, Zur Entstehung der Gasplaneten.
|
||||
Ku\SpecialChar \-
|
||||
gel\SpecialChar \-
|
||||
sym\SpecialChar \-
|
||||
me\SpecialChar \-
|
||||
tri\SpecialChar \-
|
||||
sche Gas\SpecialChar \-
|
||||
strö\SpecialChar \-
|
||||
mun\SpecialChar \-
|
||||
gen auf Pro\SpecialChar \-
|
||||
to\SpecialChar \-
|
||||
pla\SpecialChar \-
|
||||
ne\SpecialChar \-
|
||||
ten, Dissertation, Univ.
|
||||
Wien
|
||||
\layout Bibliography
|
||||
\bibitem [1979]{yorke79}
|
||||
|
||||
Yorke H.
|
||||
W., 1979, A&A 80, 215
|
||||
Terlevich, R.
|
||||
1992, in ASP Conf.
|
||||
Ser.
|
||||
31, Relationships between Active Galactic Nuclei and Starburst Galaxies,
|
||||
ed.
|
||||
A.
|
||||
V.
|
||||
Filippenko, 13
|
||||
\layout Bibliography
|
||||
\bibitem [1980a]{yorke80a}
|
||||
|
||||
Yorke H.
|
||||
W., 1980a, A&A 86, 286
|
||||
Yorke, H.
|
||||
W.
|
||||
1980a, A&A, 86, 286
|
||||
\layout Bibliography
|
||||
\bibitem [1997]{zheng}
|
||||
|
||||
Zheng, W., Davidsen, A.
|
||||
F., Tytler, D.
|
||||
& Kriss, G.
|
||||
A.
|
||||
1997, preprint
|
||||
\the_end
|
||||
@ -5,6 +5,10 @@
|
||||
#
|
||||
# 2001-05-17 take out include of stdlayouts; merge aapaper.inc
|
||||
# remove LaTeX style, rename to aa
|
||||
# 2001-05-31 Adapt to aa.cls version 5.01:
|
||||
# take out thesaurus, email -> mail
|
||||
# change layout of title
|
||||
# abstract is command
|
||||
|
||||
# General textclass parameters
|
||||
Columns 2
|
||||
@ -61,11 +65,9 @@ Style Author
|
||||
End
|
||||
Style Address
|
||||
End
|
||||
Style Email
|
||||
End
|
||||
Style Offprint
|
||||
End
|
||||
Style Thesaurus
|
||||
Style Mail
|
||||
End
|
||||
Style Date
|
||||
End
|
||||
@ -106,50 +108,31 @@ Style Subtitle
|
||||
TopSep 1.3
|
||||
BottomSep 1.3
|
||||
ParSep 1
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
Align Center
|
||||
LabelType No_Label
|
||||
|
||||
# standard font definition
|
||||
Font
|
||||
Size Normal
|
||||
Family Sans
|
||||
Size Larger
|
||||
Series Bold
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Address style definition
|
||||
Style Address
|
||||
LeftMargin MMM
|
||||
Margin Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName institute
|
||||
ParSkip 0.4
|
||||
BottomSep 0.4
|
||||
# BottomSep 0.4
|
||||
Align Left
|
||||
AlignPossible Block, Left, Right, Center
|
||||
LabelType No_Label
|
||||
|
||||
Font
|
||||
Family Sans
|
||||
Size Small
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Email address style definition
|
||||
Style Email
|
||||
Margin Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName mail
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
LeftMargin email:M
|
||||
LabelType Static
|
||||
LabelString email:
|
||||
LabelSep M
|
||||
|
||||
Font
|
||||
Family Sans
|
||||
Family Roman
|
||||
Size Small
|
||||
EndFont
|
||||
End
|
||||
@ -162,31 +145,61 @@ Style Offprint
|
||||
LatexName offprints
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
LeftMargin "Offprint Requests to:MN"
|
||||
LeftMargin "MNMOffprint Requests to:"
|
||||
LabelType Static
|
||||
LabelString "Offprint Requests to:"
|
||||
LabelSep M
|
||||
|
||||
Font
|
||||
Family Sans
|
||||
Family Roman
|
||||
Size Small
|
||||
EndFont
|
||||
LabelFont
|
||||
Family Roman
|
||||
Size Small
|
||||
Shape Slanted
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Mail address style definition
|
||||
Style Mail
|
||||
Margin Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName mail
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
LeftMargin "MJMCorrespondence to:"
|
||||
LabelType Static
|
||||
LabelString "Correspondence to:"
|
||||
LabelSep M
|
||||
|
||||
Font
|
||||
Family Roman
|
||||
Size Small
|
||||
EndFont
|
||||
LabelFont
|
||||
Family Roman
|
||||
Size Small
|
||||
Shape Slanted
|
||||
EndFont
|
||||
End
|
||||
|
||||
|
||||
# Acnowledgement style definition
|
||||
Style Acknowledgement
|
||||
Margin Static
|
||||
Margin First_Dynamic
|
||||
LatexType Environment
|
||||
LatexName acknowledgements
|
||||
NextNoIndent 1
|
||||
NextNoIndent 0
|
||||
ItemSep 0
|
||||
TopSep 0.2
|
||||
TopSep 1.2
|
||||
BottomSep 0
|
||||
ParSep 0
|
||||
Align Block
|
||||
AlignPossible Block
|
||||
LabelType Top_Environment
|
||||
LabelString Acknowledgements
|
||||
LabelType Static
|
||||
LabelString "Acknowledgements."
|
||||
LabelSep M
|
||||
# standard font definition
|
||||
Font
|
||||
@ -200,23 +213,6 @@ Style Acknowledgement
|
||||
EndFont
|
||||
End
|
||||
|
||||
Style Thesaurus
|
||||
LabelType Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName thesaurus
|
||||
NextNoIndent 1
|
||||
TopSep 0
|
||||
BottomSep 1
|
||||
LeftMargin Thesaurus:M
|
||||
LabelSep M
|
||||
LabelType Static
|
||||
LabelString Thesaurus:
|
||||
Font
|
||||
Size Small
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Caption style definition
|
||||
Style Caption
|
||||
Margin First_Dynamic
|
||||
@ -231,7 +227,6 @@ Style Caption
|
||||
LabelType Sensitive
|
||||
LabelString Caption
|
||||
|
||||
# label font definition
|
||||
LabelFont
|
||||
Series Bold
|
||||
EndFont
|
||||
@ -244,7 +239,8 @@ Style Section
|
||||
TopSep 2.0
|
||||
BottomSep 1.3
|
||||
Font
|
||||
Size Normal
|
||||
Family Sans
|
||||
Size Large
|
||||
EndFont
|
||||
End
|
||||
|
||||
@ -253,9 +249,10 @@ Style Subsection
|
||||
TopSep 1.7
|
||||
BottomSep 1.1
|
||||
Font
|
||||
Family Sans
|
||||
Series Medium
|
||||
Size Normal
|
||||
Shape Italic
|
||||
Size Large
|
||||
Shape Slanted
|
||||
EndFont
|
||||
End
|
||||
|
||||
@ -273,26 +270,29 @@ End
|
||||
Style Title
|
||||
TopSep 2
|
||||
BottomSep 1.3
|
||||
Align Left
|
||||
Align Center
|
||||
AlignPossible Left
|
||||
Font
|
||||
Family Sans
|
||||
Series Bold
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Author style redefinition
|
||||
Style Author
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
Align Center
|
||||
AlignPossible Center
|
||||
LabelType No_Label
|
||||
BottomSep 1.5
|
||||
Font
|
||||
Size Normal
|
||||
Series Bold
|
||||
Size Large
|
||||
Series Medium
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Date style redefinition
|
||||
Style Date
|
||||
LeftMargin MMM
|
||||
LabelSep ""
|
||||
TopSep 1.2
|
||||
Align Left
|
||||
@ -304,18 +304,32 @@ End
|
||||
|
||||
# Abstract style redefinition
|
||||
Style Abstract
|
||||
LeftMargin ""
|
||||
RightMargin ""
|
||||
Margin First_Dynamic
|
||||
LatexType Command
|
||||
LatexName abstract
|
||||
InTitle 1
|
||||
NextNoIndent 1
|
||||
LeftMargin MMM
|
||||
RightMargin MMM
|
||||
ParIndent ""
|
||||
TopSep 1.4
|
||||
ItemSep 0
|
||||
TopSep 1.2
|
||||
BottomSep 0.7
|
||||
LabelType Top_Environment
|
||||
ParSep 0
|
||||
Align Block
|
||||
AlignPossible Block
|
||||
LabelType static
|
||||
LabelString " Abstract "
|
||||
LabelSep M
|
||||
LabelBottomSep 0
|
||||
|
||||
Font
|
||||
Size Normal
|
||||
Size Small
|
||||
EndFont
|
||||
LabelFont
|
||||
Family Sans
|
||||
Series Bold
|
||||
Size Normal
|
||||
Size Small
|
||||
EndFont
|
||||
End
|
||||
|
||||
|
||||
134
lib/layouts/aapaper.inc
Normal file
134
lib/layouts/aapaper.inc
Normal file
@ -0,0 +1,134 @@
|
||||
# This file contains additional style definitions for the
|
||||
# A&A paper style not found in the standard include files.
|
||||
# It is Input by aapaper.layout
|
||||
#
|
||||
# Author: Peter Sütterlin <pit@uni-sw.gwdg.de>
|
||||
|
||||
# Subitle style definition
|
||||
Style Subtitle
|
||||
Margin Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName subtitle
|
||||
NextNoIndent 1
|
||||
ParSkip 0.4
|
||||
ItemSep 0
|
||||
TopSep 1.3
|
||||
BottomSep 1.3
|
||||
ParSep 1
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
LabelType No_Label
|
||||
|
||||
# standard font definition
|
||||
Font
|
||||
Size Normal
|
||||
Series Bold
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Address style definition
|
||||
Style Address
|
||||
Margin Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName institute
|
||||
ParSkip 0.4
|
||||
BottomSep 0.4
|
||||
Align Left
|
||||
AlignPossible Block, Left, Right, Center
|
||||
LabelType No_Label
|
||||
|
||||
Font
|
||||
Family Sans
|
||||
Size Small
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Email address style definition
|
||||
Style Email
|
||||
Margin Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName mail
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
LeftMargin email:M
|
||||
LabelType Static
|
||||
LabelString email:
|
||||
LabelSep M
|
||||
|
||||
Font
|
||||
Family Sans
|
||||
Size Small
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Address for Offprints style definition
|
||||
Style Offprint
|
||||
Margin Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName offprints
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
LeftMargin "Offprint Requests to:M"
|
||||
LabelType Static
|
||||
LabelString "Offprint Requests to:"
|
||||
LabelSep M
|
||||
|
||||
Font
|
||||
Family Sans
|
||||
Size Small
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Acnowledgement style definition
|
||||
Style Acknowledgement
|
||||
Margin Static
|
||||
LatexType Environment
|
||||
LatexName acknowledgements
|
||||
NextNoIndent 1
|
||||
ItemSep 0
|
||||
TopSep 0.2
|
||||
BottomSep 0
|
||||
ParSep 0
|
||||
Align Block
|
||||
AlignPossible Block
|
||||
LabelType Top_Environment
|
||||
LabelString Acknowledgements
|
||||
LabelSep M
|
||||
# standard font definition
|
||||
Font
|
||||
Size Small
|
||||
EndFont
|
||||
|
||||
# label font definition
|
||||
LabelFont
|
||||
Size Small
|
||||
Shape Italic
|
||||
EndFont
|
||||
End
|
||||
|
||||
Style Thesaurus
|
||||
LabelType Static
|
||||
LatexType Command
|
||||
InTitle 1
|
||||
LatexName thesaurus
|
||||
NextNoIndent 1
|
||||
TopSep 0
|
||||
BottomSep 1
|
||||
LeftMargin "Thesaurus not supported in recent A&A:M"
|
||||
LabelSep M
|
||||
LabelType Static
|
||||
LabelString "Thesaurus not supported in recent A&A:"
|
||||
Font
|
||||
Size Small
|
||||
EndFont
|
||||
LabelFont
|
||||
Color Red
|
||||
EndFont
|
||||
End
|
||||
|
||||
|
||||
|
||||
201
lib/layouts/aapaper.layout
Normal file
201
lib/layouts/aapaper.layout
Normal file
@ -0,0 +1,201 @@
|
||||
#% Do not delete the line below; configure depends on this
|
||||
# \DeclareLaTeXClass[aa]{article (A&A V4)}
|
||||
#
|
||||
# Author: Peter Sütterlin <pit@uni-sw.gwdg.de>
|
||||
|
||||
# This is for the old Springer layout of A&A (aa.cls version 4.x)
|
||||
# If you still have this, please upgrade to version 5 (see Extended.lyx)
|
||||
#
|
||||
# If you want to keep the layout for old papers I'd suggest to rename
|
||||
# the old style file to aa-old and change the second line in this file to
|
||||
#
|
||||
# \DeclareLaTeXClass[aa-old]{article (A&A V4)}
|
||||
#
|
||||
# and reconfigure LyX (after running texhash, of course).
|
||||
|
||||
# General textclass parameters
|
||||
Columns 2
|
||||
Sides 2
|
||||
MaxCounter Counter_Section
|
||||
SecNumDepth 3
|
||||
TocDepth 0
|
||||
PageStyle Plain
|
||||
|
||||
DefaultFont
|
||||
Family Roman
|
||||
Series Medium
|
||||
Shape Up
|
||||
Size Normal
|
||||
Color None
|
||||
EndFont
|
||||
|
||||
# Standard style definition
|
||||
Style Standard
|
||||
Margin Static
|
||||
LatexType Paragraph
|
||||
LatexName dummy
|
||||
ParIndent MM
|
||||
ParSkip 0.4
|
||||
Align Block
|
||||
AlignPossible Block, Left, Right, Center
|
||||
LabelType No_Label
|
||||
End
|
||||
|
||||
# I want to keep the entries in a logical order.
|
||||
# Therefore I'll define the entries first, then fill them
|
||||
|
||||
Style Itemize
|
||||
End
|
||||
Style Enumerate
|
||||
End
|
||||
Style Description
|
||||
End
|
||||
Style List
|
||||
End
|
||||
Style Caption
|
||||
End
|
||||
Style LaTeX
|
||||
End
|
||||
Style Section
|
||||
End
|
||||
Style Subsection
|
||||
End
|
||||
Style Subsubsection
|
||||
End
|
||||
Style Title
|
||||
End
|
||||
Style Subtitle
|
||||
End
|
||||
Style Author
|
||||
End
|
||||
Style Address
|
||||
End
|
||||
Style Email
|
||||
End
|
||||
Style Offprint
|
||||
End
|
||||
Style Thesaurus
|
||||
End
|
||||
Style Date
|
||||
End
|
||||
Style Abstract
|
||||
End
|
||||
Style Acknowledgement
|
||||
End
|
||||
Style Bibliography
|
||||
End
|
||||
|
||||
# OK, now we have a more or less consistent Ordering. Now fill the
|
||||
# definitions.
|
||||
# First, the standard includes
|
||||
|
||||
Input stdlists.inc
|
||||
Input stdlayouts.inc
|
||||
Input stdsections.inc
|
||||
Input stdtitle.inc
|
||||
Input stdstruct.inc
|
||||
|
||||
# Remove unwanted Styles
|
||||
|
||||
NoStyle Quotation
|
||||
NoStyle Quote
|
||||
NoStyle Verse
|
||||
NoStyle Chapter
|
||||
NoStyle Paragraph
|
||||
NoStyle Subparagraph
|
||||
NoStyle Part
|
||||
|
||||
# Definitions only valid for A&A style
|
||||
Input aapaper.inc
|
||||
|
||||
# Redefine some things
|
||||
|
||||
# Section style redefinition
|
||||
Style Section
|
||||
TopSep 2.0
|
||||
BottomSep 1.3
|
||||
Font
|
||||
Size Normal
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Subsection style redefinition
|
||||
Style Subsection
|
||||
TopSep 1.7
|
||||
BottomSep 1.1
|
||||
Font
|
||||
Series Medium
|
||||
Size Normal
|
||||
Shape Italic
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Subsubsection style redefinition
|
||||
Style Subsubsection
|
||||
TopSep 1.7
|
||||
BottomSep 1.1
|
||||
Font
|
||||
Series Medium
|
||||
Size Normal
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Title style redefinition
|
||||
Style Title
|
||||
TopSep 2
|
||||
BottomSep 1.3
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
Font
|
||||
Series Bold
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Author style redefinition
|
||||
Style Author
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
LabelType No_Label
|
||||
Font
|
||||
Size Normal
|
||||
Series Bold
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Date style redefinition
|
||||
Style Date
|
||||
LabelSep ""
|
||||
TopSep 1.2
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
Font
|
||||
Size Small
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Abstract style redefinition
|
||||
Style Abstract
|
||||
LeftMargin ""
|
||||
RightMargin ""
|
||||
ParIndent ""
|
||||
TopSep 1.4
|
||||
BottomSep 0.7
|
||||
LabelType Top_Environment
|
||||
Font
|
||||
Size Normal
|
||||
EndFont
|
||||
LabelFont
|
||||
Series Bold
|
||||
Size Normal
|
||||
EndFont
|
||||
End
|
||||
|
||||
# Bibliography style redefinition
|
||||
Style Bibliography
|
||||
Align Left
|
||||
AlignPossible Left
|
||||
LabelFont
|
||||
Series Bold
|
||||
EndFont
|
||||
End
|
||||
|
||||
@ -1,12 +1,13 @@
|
||||
#This file was created by <pit> Mon Nov 24 23:26:21 1997
|
||||
#LyX 0.11 (C) 1995-1997 Matthias Ettrich and the LyX Team
|
||||
\lyxformat 2.15
|
||||
#LyX 1.1 created this file. For more info see http://www.lyx.org/
|
||||
\lyxformat 218
|
||||
\textclass aa
|
||||
\language english
|
||||
\inputencoding auto
|
||||
\fontscheme times
|
||||
\graphics default
|
||||
\paperfontsize default
|
||||
\spacing single
|
||||
\papersize Default
|
||||
\paperpackage a4
|
||||
\use_geometry 0
|
||||
\use_amsmath 0
|
||||
@ -15,13 +16,12 @@
|
||||
\tocdepth 3
|
||||
\paragraph_separation indent
|
||||
\defskip medskip
|
||||
\quotes_language english
|
||||
\quotes_times 2
|
||||
\papercolumns 2
|
||||
\papersides 2
|
||||
\paperpagestyle default
|
||||
|
||||
\layout Thesaurus
|
||||
|
||||
Put the Thesaurus codes here
|
||||
\layout Title
|
||||
|
||||
This is your Title
|
||||
@ -54,29 +54,45 @@ inst{
|
||||
\layout Address
|
||||
|
||||
Here
|
||||
\newline
|
||||
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
email{
|
||||
\latex default
|
||||
myaddress
|
||||
\latex latex
|
||||
}
|
||||
\newline
|
||||
|
||||
\backslash
|
||||
and
|
||||
\latex default
|
||||
There
|
||||
\layout Offprint
|
||||
\newline
|
||||
|
||||
Me
|
||||
\layout Email
|
||||
\latex latex
|
||||
|
||||
\backslash
|
||||
email{
|
||||
\latex default
|
||||
youraddress
|
||||
\latex latex
|
||||
}
|
||||
\layout Offprint
|
||||
|
||||
Me
|
||||
\layout Date
|
||||
|
||||
Received / Accepted
|
||||
Received ; Accepted
|
||||
\layout Abstract
|
||||
|
||||
Short abstract
|
||||
\layout Abstract
|
||||
|
||||
|
||||
\latex latex
|
||||
|
||||
\newline
|
||||
|
||||
\backslash
|
||||
keywords{
|
||||
\latex default
|
||||
|
||||
Loading…
Reference in New Issue
Block a user