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aa class changes from Pit

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git-svn-id: svn://svn.lyx.org/lyx/lyx-devel/trunk@2115 a592a061-630c-0410-9148-cb99ea01b6c8
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Jean-Marc Lasgouttes 2001-06-13 13:45:51 +00:00
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lib/ChangeLog
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@ -1,3 +1,17 @@
2001-06-12 Peter Suetterlin <P.Suetterlin@astro.uu.nl>
* examples/aa_head.lyx:
* examples/aa_paper.lyx: removed
* doc/LaTeXConfig.lyx.in:
* examples/aa_sample.lyx:
* layouts/aa.layout:
* layouts/aapaper.inc:
* layouts/aapaper.layout:
* templates/aa.lyx: aa.layout is for the new version of the
A&A document class, while aapaper.layout is for the older (and
slightly incompatible) version.
2001-06-07 Jean-Marc Lasgouttes <Jean-Marc.Lasgouttes@inria.fr> 2001-06-07 Jean-Marc Lasgouttes <Jean-Marc.Lasgouttes@inria.fr>
* doc/LaTeXConfig.lyx.in: * doc/LaTeXConfig.lyx.in:
@ -24,12 +38,12 @@
2001-05-22 Adrien Rebollo <rebollo@iaf.cnrs-gif.fr> 2001-05-22 Adrien Rebollo <rebollo@iaf.cnrs-gif.fr>
* lib/kbd/european.kmap: * kbd/european.kmap:
* lib/kbd/francais.kmap: * kbd/francais.kmap:
* lib/kbd/iso8859-15.cdef: * kbd/iso8859-15.cdef:
* encodings: add iso8859-15 support. * encodings: add iso8859-15 support.
* lib/kbd/iso8859-1.cdef: cleanup * kbd/iso8859-1.cdef: cleanup
2001-05-22 Peter Suetterlin <P.Suetterlin@astro.uu.nl> 2001-05-22 Peter Suetterlin <P.Suetterlin@astro.uu.nl>

17
lib/doc/LaTeXConfig.lyx.in
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@ -360,16 +360,16 @@ Additional document classes
aa aa
\layout Description \layout Description
Found: @chk_aapaper@ Found: @chk_aa@
\layout Description \layout Description
CTAN: N/A (available from Springer's ftp site CTAN: N/A (available from ftp site
\family typewriter \family typewriter
ftp.springer.de ftp.edpsciences.org
\family default \family default
in directory in directory
\family typewriter \family typewriter
/pub/tex/latex/aa /pub/aa/
\family default \family default
) )
\layout Description \layout Description
@ -378,16 +378,13 @@ Notes: The document class
\family sans \family sans
aa aa
\family default \family default
can be used to write articles for submission to the scientific journal (Version 5.01) can be used to write articles for submission to the
scientific journal
\emph on \emph on
Astronomy and Astrophysics Astronomy and Astrophysics
\emph default \emph default
and the accompanying published by EDP Sciences.
\emph on
Supplement Series
\emph default
published by Springer -Verlag.
\layout Subsection \layout Subsection
aastex aastex

153
lib/examples/aa_head.lyx
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@ -1,153 +0,0 @@
#This file was created by <pit> Tue Nov 25 23:06:48 1997
#LyX 0.11 (C) 1995-1997 Matthias Ettrich and the LyX Team
\lyxformat 2.15
\textclass aa
\language english
\inputencoding latin1
\fontscheme times
\graphics default
\paperfontsize default
\spacing single
\papersize Default
\paperpackage a4
\use_geometry 0
\use_amsmath 0
\paperorientation portrait
\secnumdepth 3
\tocdepth 3
\paragraph_separation indent
\defskip medskip
\quotes_language english
\quotes_times 2
\papercolumns 2
\papersides 2
\paperpagestyle default
\layout Thesaurus
Sorry, no thesaurus for that
\layout Title
The Use of LyX in Astronomy
\layout Subtitle
Looking towards a bright future
\layout Author
P.
Sütterlin
\latex latex
\backslash
inst{
\latex default
1
\latex latex
}
\begin_float footnote
\layout Standard
\series medium
\emph on
Present Address:
\emph default
Universitäts-Sternwarte, Geismarlandstr.
11, D-37083 Göttingen
\end_float
\latex latex
\backslash
and
\latex default
A.N.
Coauthor
\latex latex
\backslash
inst{
\latex default
2
\latex latex
}
\layout Address
Kiepenheuer-Institut für Sonnenphysik, Schöneckstr.
6, D-79104 Freiburg
\latex latex
\backslash
and
\latex default
Somewhere-in-the-Country
\layout Offprint
P.
Sütterlin
\layout Email
pit@uni-sw.gwdg.de
\layout Date
Received: maybe / Accepted: who knows
\layout Abstract
In this paper we show that LyX can be used to write papers for puplication
in the journal Astronomy and Astrophysics.
\layout Abstract
\latex latex
\backslash
keywords{
\latex default
LaTeX - Wordprocessing - Publication
\latex latex
}
\layout Section
Intoduction
\layout Standard
In 1997, Springer Verlag decided to accept papers for publication in their
journals
\emph on
Astronomy and Astrophysics
\emph default
and the acompanying
\emph on
Supplement Series
\emph default
only in form of LaTeX.
At the same time, they switched the layout macros to LaTeX2
\begin_inset Formula \( \epsilon \)
\end_inset
(Lamport
\begin_inset LatexCommand \cite{kopka}
\end_inset
).
This made it easy to adapt a corresponding LyX style to produce the correct
output for direct submission to A&A.
\layout Section
Discussion
\layout Standard
What is there to discuss about? The existence of LyX with this layout makes
it as easy as one could wish to write scientific papers.
\layout Bibliography
\bibitem [1994]{lamport}
L.
Lamport, 1994:
\emph on
LaTeX: A Document Preparation System
\emph default
, Addison-Wesley Publishing Company, 2nd edition
\the_end

418
lib/examples/aa_paper.lyx → lib/examples/aa_sample.lyx
View File

@ -1,8 +1,12 @@
#LyX 1.1 created this file. For more info see http://www.lyx.org/ #LyX 1.1 created this file. For more info see http://www.lyx.org/
\lyxformat 218 \lyxformat 218
\textclass aa \textclass aa
\begin_preamble
\usepackage{graphicx}
%
\end_preamble
\language english \language english
\inputencoding latin1 \inputencoding auto
\fontscheme default \fontscheme default
\graphics default \graphics default
\paperfontsize default \paperfontsize default
@ -22,9 +26,6 @@
\papersides 2 \papersides 2
\paperpagestyle default \paperpagestyle default
\layout Thesaurus
06(03.11.1;16.06.1;19.06.1;19.37.1;19.53.1;19.63.1)
\layout Title \layout Title
Hydrodynamics of giant planet formation Hydrodynamics of giant planet formation
@ -40,20 +41,67 @@ I.
G. G.
Wuchterl Wuchterl
\layout Address \latex latex
\backslash
inst{1}
\backslash
and
\newline
\latex default
C.
Ptolemy
\latex latex
\backslash
inst{2}
\backslash
fnmsep
\begin_float footnote
\layout Standard
Just to show the usage of the elements in the author field
\end_float
Institute for Astronomy (IfA), University of Vienna, Türkenschanzstrasse
17, A-1180 Vienna
\layout Offprint \layout Offprint
G. G.
Wuchterl Wuchterl
\layout Email \layout Address
Institute for Astronomy (IfA), University of Vienna, T\i \"{u}
rkenschanzstrasse
17, A-1180 Vienna
\newline
\latex latex
\backslash
email{wuchterl@amok.ast.univie.ac.at}
\backslash
and
\newline
\latex default
University of Alexandria, Department of Geography, ...
\newline
\latex latex
\backslash
email{c.ptolemy@hipparch.uheaven.space}
\latex default
\begin_float footnote
\layout Standard
The university of heaven temporarily does not accept e-mails
\end_float
wuchterl@amok.ast.univie.ac.at
\layout Date \layout Date
Received September 15, 1996 / Accepted March 16, 1997 Received September 15, 1996; accepted March 16, 1997
\layout Abstract \layout Abstract
To investigate the physical nature of the `nuc\SpecialChar \- To investigate the physical nature of the `nuc\SpecialChar \-
@ -74,8 +122,6 @@ leated instability' of proto
opacities and the local thermodynamic state in the layer. opacities and the local thermodynamic state in the layer.
Stability and instability can therefore be expressed in the form of stability Stability and instability can therefore be expressed in the form of stability
equations of state which are universal for a given composition. equations of state which are universal for a given composition.
\layout Abstract
The stability equations of state are calculated for solar composition and The stability equations of state are calculated for solar composition and
are displayed in the domain are displayed in the domain
\begin_inset Formula \( -14\leq \lg \rho /[\mathrm{g}\, \mathrm{cm}^{-3}]\leq 0 \) \begin_inset Formula \( -14\leq \lg \rho /[\mathrm{g}\, \mathrm{cm}^{-3}]\leq 0 \)
@ -103,7 +149,7 @@ The stability equations of state are calculated for solar composition and
. .
Regions of instability in the Regions of instability in the
\begin_inset Formula \( (\rho \, e) \) \begin_inset Formula \( (\rho ,e) \)
\end_inset \end_inset
-plane are described and related to the underlying microphysical processes. -plane are described and related to the underlying microphysical processes.
@ -114,21 +160,20 @@ The stability equations of state are calculated for solar composition and
\end_inset \end_inset
-mechanism is widespread under `cool' conditions. -mechanism is widespread under `cool' conditions.
\layout Abstract
\latex latex \latex latex
\newline
\backslash \backslash
keywords{ keywords{giant planet formation --
\backslash
(
\backslash
kappa
\backslash
)-mechanism -- stability of gas spheres }
\latex default \latex default
giant planet formation --
\begin_inset Formula \( \kappa \)
\end_inset
-mechanism -- stability of gas spheres
\latex latex
}
\layout Section \layout Section
Introduction Introduction
@ -137,7 +182,12 @@ Introduction
In the In the
\emph on \emph on
nucleated instability nucleated instability
\latex latex
\backslash
/{}
\emph default \emph default
\latex default
(also called core instability) hypothesis of giant planet formation, a (also called core instability) hypothesis of giant planet formation, a
critical mass for static core envelope protoplanets has been found. critical mass for static core envelope protoplanets has been found.
Mizuno ( Mizuno (
@ -171,37 +221,12 @@ Although no hydrodynamical study has been available many workers conjectured
\end_inset \end_inset
) standard one-zone model. ) standard one-zone model.
The nonlinear, hydrodynamic evolution of the protogiant planet beyond the
critical mass, as calculated by Wuchterl (
\begin_inset LatexCommand \cite{wuchterl}
\end_inset
), will be described in a forthcoming article.
\layout Standard
The fact that Wuchterl (
\begin_inset LatexCommand \cite{wuchterl}
\end_inset
) found the excitation of hydrodynamical waves in his models raises considerable
interest on the transition from static to dynamic evolutionary phases of
the protogiant planet at the critical mass.
The waves play a crucial role in the development of the so-called nucleated
instability in the nucleated instability hypothesis.
They lead to the formation of shock waves and massive outflow phenomena.
The protoplanet evolves into a new quasi-equilibrium structure with a
\emph on
pulsating
\emph default
envelope, after the mass loss phase has declined.
\layout Standard \layout Standard
Phenomena similar to the ones described above for giant planet formation Phenomena similar to the ones described above for giant planet formation
have been found in hydrodynamical models concerning star formation where have been found in hydrodynamical models concerning star formation where
protostellar cores explode (Tscharnuter protostellar cores explode (Tscharnuter
\begin_inset LatexCommand \cite{tscarnuter} \begin_inset LatexCommand \cite{tscharnuter}
\end_inset \end_inset
@ -220,21 +245,10 @@ Baker's standard one-zone model
\layout Standard \layout Standard
\begin_float wide-fig \begin_float wide-fig
\layout Standard
\latex latex
\backslash
rule{0.4pt}{4cm}
\hfill
\backslash
parbox[b]{55mm}{
\layout Caption \layout Caption
Adiabatic exponent Adiabatic exponent
\begin_inset Formula \( \Gamma \) \begin_inset Formula \( \Gamma _{1} \)
\end_inset \end_inset
. .
@ -259,20 +273,22 @@ is plotted as a function of
\end_inset \end_inset
\layout Standard
\begin_inset LatexCommand \label{FigGam} \begin_inset LatexCommand \label{FigGam}
\end_inset \end_inset
\latex latex
}
\end_float \end_float
In this section the one-zone model of Baker ( In this section the one-zone model of Baker (
\begin_inset LatexCommand \cite{baker} \begin_inset LatexCommand \cite{baker}
\end_inset \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. reviewed.
The resulting stability criteria will be rewritten in terms of local state The resulting stability criteria will be rewritten in terms of local state
variables, local timescales and constitutive relations. variables, local timescales and constitutive relations.
@ -294,10 +310,16 @@ thermal equilibrium,
\layout Itemize \layout Itemize
energy transport by grey radiation diffusion. energy transport by grey radiation diffusion.
\layout Standard
\layout Standard
\noindent
For the one-zone-model Baker obtains necessary conditions for dynamical, 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, (34a,
\latex latex \latex latex
@ -315,24 +337,35 @@ c) in Baker
\end_inset \end_inset
]. ).
Using Baker's notation: Using Baker's notation:
\layout Standard
\align left
\begin_inset Formula \begin{eqnarray*} \begin_inset Formula \begin{eqnarray*}
M_{\mathrm{r}} & & \mathrm{mass}\, \mathrm{internal}\, \mathrm{to}\, \mathrm{the}\, \mathrm{radius}\, r\\ M_{r} & & \textrm{mass internal to the radius }r\\
m & & \mathrm{mass}\, \mathrm{of}\, \mathrm{the}\, \mathrm{zone}\\ m & & \textrm{mass of the zone}\\
r_{0} & & \mathrm{unperturbed}\, \mathrm{zone}\, \mathrm{radius}\\ r_{0} & & \textrm{unperturbed zone radius}\\
\rho _{0} & & \mathrm{unperturbed}\, \mathrm{density}\, \mathrm{in}\, \mathrm{the}\, \mathrm{zone}\\ \rho _{0} & & \textrm{unperturbed density in the zone}\\
T_{0} & & \mathrm{unperturbed}\, \mathrm{temperature}\, \mathrm{in}\, \mathrm{the}\, \mathrm{zone}\\ T_{0} & & \textrm{unperturbed temperature in the zone}\\
L_{r0} & & \mathrm{unperturbed}\, \mathrm{luminosity}\\ L_{r0} & & \textrm{unperturbed luminosity}\\
E_{\mathrm{th}} & & \mathrm{thermal}\, \mathrm{energy}\, \mathrm{of}\, \mathrm{the}\, \mathrm{zone} E_{\textrm{th}} & & \textrm{thermal energy of the zone}
\end{eqnarray*} \end{eqnarray*}
\end_inset \end_inset
\layout Standard
\noindent
and with the definitions of the and with the definitions of the
\emph on \emph on
local cooling time local cooling time
\latex latex
\backslash
/{}
\emph default \emph default
\latex default
(see Fig.\SpecialChar ~ (see Fig.\SpecialChar ~
\begin_inset LatexCommand \ref{FigGam} \begin_inset LatexCommand \ref{FigGam}
@ -340,9 +373,6 @@ local cooling time
\end_inset \end_inset
) )
\layout Standard
\begin_inset Formula \begin{equation} \begin_inset Formula \begin{equation}
\tau _{\mathrm{co}}=\frac{E_{\mathrm{th}}}{L_{r0}}\, , \tau _{\mathrm{co}}=\frac{E_{\mathrm{th}}}{L_{r0}}\, ,
\end{equation} \end{equation}
@ -352,11 +382,10 @@ local cooling time
and the and the
\emph on \emph on
local free-fall time local free-fall time
\layout Standard \emph default
\begin_inset Formula \begin{equation} \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{equation}
\end_inset \end_inset
@ -378,13 +407,10 @@ K & = & \frac{\sqrt{32}}{\pi }\frac{1}{\delta }\frac{\tau _{\mathrm{ff}}}{\tau _
\end_inset \end_inset
where where
\begin_inset Formula \( E_{\mathrm{th}}\approx m(P_{0}/\rho _{0}) \) \begin_inset Formula \( E_{\mathrm{th}}\approx m(P_{0}/{\rho _{0}}) \)
\end_inset \end_inset
has been used and has been used and
\layout Standard
\begin_inset Formula \begin{equation} \begin_inset Formula \begin{equation}
\begin{array}{l} \begin{array}{l}
\delta =-\left( \frac{\partial \ln \rho }{\partial \ln T}\right) _{P}\\ \delta =-\left( \frac{\partial \ln \rho }{\partial \ln T}\right) _{P}\\
@ -425,31 +451,30 @@ is a thermodynamical quantity which is of order
Substituting into Baker's criteria, using thermodynamic identities and Substituting into Baker's criteria, using thermodynamic identities and
definitions of thermodynamic quantities, definitions of thermodynamic quantities,
\begin_inset Formula \[ \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 \end_inset
\layout Standard
\begin_inset Formula \[ \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 \end_inset
one obtains, after some pages of algebra, the conditions for one obtains, after some pages of algebra, the conditions for
\emph on \emph on
stability stability
\latex latex
\backslash
/{}
\emph default \emph default
\latex default
given below: given below:
\layout Standard
\begin_inset Formula \begin{eqnarray} \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}}{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}}{\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}}{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{eqnarray}
\end_inset \end_inset
@ -475,6 +500,7 @@ a factor containing local timescales only,
\layout Enumerate \layout Enumerate
a factor containing only constitutive relations and their derivatives. a factor containing only constitutive relations and their derivatives.
\layout Standard \layout Standard
The first factors, depending on only timescales, are positive by definition. The first factors, depending on only timescales, are positive by definition.
@ -505,6 +531,11 @@ functions of the thermodynamic state in the local zone
The one-zone stability can therefore be determined from a simple equation The one-zone stability can therefore be determined from a simple equation
of state, given for example, as a function of density and temperature. of state, given for example, as a function of density and temperature.
Once the microphysics, i.e. Once the microphysics, i.e.
\latex latex
\backslash
\latex default
the thermodynamics and opacities (see Table\SpecialChar ~ the thermodynamics and opacities (see Table\SpecialChar ~
\begin_inset LatexCommand \ref{KapSou} \begin_inset LatexCommand \ref{KapSou}
@ -523,12 +554,12 @@ functions of the thermodynamic state in the local zone
\begin_float tab \begin_float tab
\layout Caption \layout Caption
Opacity sources
\begin_inset LatexCommand \label{KapSou} \begin_inset LatexCommand \label{KapSou}
\end_inset \end_inset
Opacity sources
\layout Standard \layout Standard
@ -537,7 +568,7 @@ Opacity sources
<features rotate="false" islongtable="false" endhead="0" endfirsthead="0" endfoot="0" endlastfoot="0"> <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="">
<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=""> <cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="false" rotate="false" usebox="none" width="" special="">
\begin_inset Text \begin_inset Text
@ -546,16 +577,20 @@ Opacity sources
Source Source
\end_inset \end_inset
</cell> </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 \begin_inset Text
\layout Standard \layout Standard
T/[K]
\begin_inset Formula \( T/[\textrm{K}] \)
\end_inset
\end_inset \end_inset
</cell> </cell>
</row> </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=""> <cell multicolumn="0" alignment="center" valignment="top" topline="true" bottomline="false" leftline="true" rightline="false" rotate="false" usebox="none" width="" special="">
\begin_inset Text \begin_inset Text
@ -564,13 +599,13 @@ T/[K]
Yorke 1979, Yorke 1980a Yorke 1979, Yorke 1980a
\end_inset \end_inset
</cell> </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 \begin_inset Text
\layout Standard \layout Standard
\begin_inset Formula \( \leq 1700^{\mathrm{a}} \) \begin_inset Formula \( \leq 1700^{\textrm{a}} \)
\end_inset \end_inset
@ -586,7 +621,7 @@ Yorke 1979, Yorke 1980a
Krügel 1971 Krügel 1971
\end_inset \end_inset
</cell> </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 \begin_inset Text
\layout Standard \layout Standard
@ -608,7 +643,7 @@ Kr
Cox & Stewart 1969 Cox & Stewart 1969
\end_inset \end_inset
</cell> </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 \begin_inset Text
\layout Standard \layout Standard
@ -627,30 +662,13 @@ Cox & Stewart 1969
\layout Standard \layout Standard
\added_space_top medskip*
\begin_inset Formula \( ^{\textrm{a}} \) \begin_inset Formula \( ^{\textrm{a}} \)
\end_inset \end_inset
This is footnote a This is footnote a
\end_float \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 ( of the left-hand sides of the inequalities (
\begin_inset LatexCommand \ref{ZSDynSta} \begin_inset LatexCommand \ref{ZSDynSta}
@ -685,40 +703,31 @@ The sign determining part of inequality\SpecialChar ~
\end_inset \end_inset
and it reduces to the criterion for dynamical stability and it reduces to the criterion for dynamical stability
\layout Standard
\begin_inset Formula \begin{equation} \begin_inset Formula \begin{equation}
\Gamma _{1}>\frac{4}{3} \Gamma _{1}>\frac{4}{3}\, \cdot
\end{equation} \end{equation}
\end_inset \end_inset
Stability of the thermodynamical equilibrium demands Stability of the thermodynamical equilibrium demands
\begin_inset Formula \begin{equation} \begin_inset Formula \begin{equation}
\chi _{\rho }>0,\: \: c_{v}>0\, , \chi ^{}_{\rho }>0,\; \; c_{v}>0\, ,
\end{equation} \end{equation}
\end_inset \end_inset
and and
\layout Standard
\begin_inset Formula \begin{equation} \begin_inset Formula \begin{equation}
\chi _{T}>0 \chi ^{}_{T}>0
\end{equation} \end{equation}
\end_inset \end_inset
holds for a wide range of physical situations. holds for a wide range of physical situations.
With With
\layout Standard
\begin_inset Formula \begin{eqnarray} \begin_inset Formula \begin{eqnarray}
\Gamma _{3}-1=\frac{P}{\rho T}\frac{\chi _{T}}{c_{v}} & > & 0\\ \Gamma _{3}-1=\frac{P}{\rho T}\frac{\chi ^{}_{T}}{c_{v}} & > & 0\\
\Gamma _{1}=\chi _{\rho }+\chi _{T}(\Gamma _{3}-1) & > & 0\\ \Gamma _{1}=\chi _{\rho }^{}+\chi _{T}^{}(\Gamma _{3}-1) & > & 0\\
\nabla _{\mathrm{ad}}=\frac{\Gamma _{3}-1}{\Gamma _{1}} & > & 0 \nabla _{\mathrm{ad}}=\frac{\Gamma _{3}-1}{\Gamma _{1}} & > & 0
\end{eqnarray} \end{eqnarray}
@ -741,19 +750,16 @@ we find the sign determining terms in inequalities\SpecialChar ~
stability stability
\emph default \emph default
, respectively: , respectively:
\layout Standard
\begin_inset Formula \begin{eqnarray} \begin_inset Formula \begin{eqnarray}
3\Gamma _{1}-4=:\, S_{\mathrm{dyn}}> & 0 & \label{DynSta} \\ 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} \\ \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} 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{eqnarray}
\end_inset \end_inset
The constitutive relations are to be evaluated for the unperturbed thermodynamic The constitutive relations are to be evaluated for the unperturbed thermodynami
state (say c state (say
\begin_inset Formula \( (\rho _{0},T_{0}) \) \begin_inset Formula \( (\rho _{0},T_{0}) \)
\end_inset \end_inset
@ -768,11 +774,11 @@ e relations
\end_inset \end_inset
, ,
\begin_inset Formula \( \chi _{T},\, \chi _{\rho } \) \begin_inset Formula \( \chi _{T}^{},\, \chi _{\rho }^{} \)
\end_inset \end_inset
, ,
\begin_inset Formula \( \kappa _{P},\, \kappa _{T} \) \begin_inset Formula \( \kappa _{P}^{},\, \kappa _{T}^{} \)
\end_inset \end_inset
. .
@ -799,22 +805,10 @@ e relations
. .
Regions of secular instability are listed in Table\SpecialChar ~ Regions of secular instability are listed in Table\SpecialChar ~
1.
\begin_inset LatexCommand \ref{TabSecInst}
\end_inset
.
\layout Standard \layout Standard
\begin_float fig \begin_float fig
\layout Standard
\latex latex
\backslash
vspace{5cm}
\layout Caption \layout Caption
Vibrational stability equation of state Vibrational stability equation of state
@ -826,7 +820,10 @@ Vibrational stability equation of state
\begin_inset Formula \( >0 \) \begin_inset Formula \( >0 \)
\end_inset \end_inset
means vibrational stability. means vibrational stability
\layout Standard
\begin_inset LatexCommand \label{FigVibStab} \begin_inset LatexCommand \label{FigVibStab}
\end_inset \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. ) standard one-zone model, can be expressed as stability equations of state.
These stability equations of state depend only on the local thermodynamic These stability equations of state depend only on the local thermodynamic
state of the layer. state of the layer.
\layout Enumerate \layout Enumerate
If the constitutive relations -- equations of state and Rosseland mean opacities If the constitutive relations -- equations of state and Rosseland mean opacities
-- are specified, the stability equations of state can be evaluated without -- are specified, the stability equations of state can be evaluated without
specifying properties of the layer. specifying properties of the layer.
\layout Enumerate \layout Enumerate
For solar composition gas the 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 dissociation and the combined H, first He ionization zone, as indicated
by vibrational instability. by vibrational instability.
These regions of instability are much larger in extent and degree of instabilit 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 \layout Acknowledgement
Part of this work was supported by the German Part of this work was supported by the German
@ -877,81 +878,86 @@ schungs\SpecialChar \-
ge\SpecialChar \- ge\SpecialChar \-
mein\SpecialChar \- mein\SpecialChar \-
schaft, DFG schaft, DFG
\latex latex
\backslash
/{}
\emph default \emph default
\latex default
project number Ts\SpecialChar ~ project number Ts\SpecialChar ~
17/2--1. 17/2--1.
\layout Bibliography \layout Bibliography
\bibitem [1966]{baker} \bibitem [1966]{baker}
Baker N., 1966, in: Stellar Evolution, eds.\SpecialChar ~ Baker, N.
1966, in Stellar Evolution, ed.
\latex latex
\backslash
\latex default
R. R.
F. F.
Stein, A. Stein,& A.
G. G.
W. W.
Cameron, Plenum, New York, p.\SpecialChar ~ Cameron (Plenum, New York) 333
333
\layout Bibliography \layout Bibliography
\bibitem [1988]{balluch} \bibitem [1988]{balluch}
Balluch M., 1988, A&A 200, 58 Balluch, M.
1988, A&A, 200, 58
\layout Bibliography \layout Bibliography
\bibitem [1980]{cox} \bibitem [1980]{cox}
Cox J. Cox, J.
P., 1980, Theory of Stellar Pulsation, Princeton University Press, Princeton, P.
p.\SpecialChar ~ 1980, Theory of Stellar Pulsation (Princeton University Press, Princeton)
165 165
\layout Bibliography \layout Bibliography
\bibitem [1969]{cox69} \bibitem [1969]{cox69}
Cox A. Cox, A.
N., Stewart J. N.,& Stewart, J.
N., 1969, Academia Nauk, Scientific Information 15, 1 N.
\layout Bibliography 1969, Academia Nauk, Scientific Information 15, 1
\bibitem [1971]{kruegel}
Krügel E., 1971, Der Rosselandsche Mittelwert bei tiefen Temperaturen, Diplom--Th
esis, Univ.\SpecialChar ~
Göttingen
\layout Bibliography \layout Bibliography
\bibitem [1980]{mizuno} \bibitem [1980]{mizuno}
Mizuno H., 1980, Prog. Mizuno H.
1980, Prog.
Theor. Theor.
Phys. Phys., 64, 544
64, 544
\layout Bibliography \layout Bibliography
\bibitem [1987]{tscarnuter} \bibitem [1987]{tscharnuter}
Tscharnuter W. Tscharnuter W.
M., 1987, A&A 188, 55 M.
1987, A&A, 188, 55
\layout Bibliography \layout Bibliography
\bibitem [1989]{wuchterl} \bibitem [1992]{terlevich}
Wuchterl G., 1989, Zur Entstehung der Gasplaneten. Terlevich, R.
Ku\SpecialChar \- 1992, in ASP Conf.
gel\SpecialChar \- Ser.
sym\SpecialChar \- 31, Relationships between Active Galactic Nuclei and Starburst Galaxies,
me\SpecialChar \- ed.
tri\SpecialChar \- A.
sche Gas\SpecialChar \- V.
strö\SpecialChar \- Filippenko, 13
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
\layout Bibliography \layout Bibliography
\bibitem [1980a]{yorke80a} \bibitem [1980a]{yorke80a}
Yorke H. Yorke, H.
W., 1980a, A&A 86, 286 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 \the_end

148
lib/layouts/aa.layout
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@ -5,6 +5,10 @@
# #
# 2001-05-17 take out include of stdlayouts; merge aapaper.inc # 2001-05-17 take out include of stdlayouts; merge aapaper.inc
# remove LaTeX style, rename to aa # 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 # General textclass parameters
Columns 2 Columns 2
@ -61,11 +65,9 @@ Style Author
End End
Style Address Style Address
End End
Style Email
End
Style Offprint Style Offprint
End End
Style Thesaurus Style Mail
End End
Style Date Style Date
End End
@ -106,50 +108,31 @@ Style Subtitle
TopSep 1.3 TopSep 1.3
BottomSep 1.3 BottomSep 1.3
ParSep 1 ParSep 1
Align Left Align Center
AlignPossible Left
LabelType No_Label LabelType No_Label
# standard font definition # standard font definition
Font Font
Size Normal Family Sans
Size Larger
Series Bold Series Bold
EndFont EndFont
End End
# Address style definition # Address style definition
Style Address Style Address
LeftMargin MMM
Margin Static Margin Static
LatexType Command LatexType Command
InTitle 1 InTitle 1
LatexName institute LatexName institute
ParSkip 0.4 ParSkip 0.4
BottomSep 0.4 # BottomSep 0.4
Align Left Align Left
AlignPossible Block, Left, Right, Center
LabelType No_Label LabelType No_Label
Font Font
Family Sans Family Roman
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 Size Small
EndFont EndFont
End End
@ -162,31 +145,61 @@ Style Offprint
LatexName offprints LatexName offprints
Align Left Align Left
AlignPossible Left AlignPossible Left
LeftMargin "Offprint Requests to:MN" LeftMargin "MNMOffprint Requests to:"
LabelType Static LabelType Static
LabelString "Offprint Requests to:" LabelString "Offprint Requests to:"
LabelSep M LabelSep M
Font Font
Family Sans Family Roman
Size Small Size Small
EndFont EndFont
LabelFont
Family Roman
Size Small
Shape Slanted
EndFont
End 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 # Acnowledgement style definition
Style Acknowledgement Style Acknowledgement
Margin Static Margin First_Dynamic
LatexType Environment LatexType Environment
LatexName acknowledgements LatexName acknowledgements
NextNoIndent 1 NextNoIndent 0
ItemSep 0 ItemSep 0
TopSep 0.2 TopSep 1.2
BottomSep 0 BottomSep 0
ParSep 0 ParSep 0
Align Block Align Block
AlignPossible Block AlignPossible Block
LabelType Top_Environment LabelType Static
LabelString Acknowledgements LabelString "Acknowledgements."
LabelSep M LabelSep M
# standard font definition # standard font definition
Font Font
@ -200,23 +213,6 @@ Style Acknowledgement
EndFont EndFont
End 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 # Caption style definition
Style Caption Style Caption
Margin First_Dynamic Margin First_Dynamic
@ -231,7 +227,6 @@ Style Caption
LabelType Sensitive LabelType Sensitive
LabelString Caption LabelString Caption
# label font definition
LabelFont LabelFont
Series Bold Series Bold
EndFont EndFont
@ -244,7 +239,8 @@ Style Section
TopSep 2.0 TopSep 2.0
BottomSep 1.3 BottomSep 1.3
Font Font
Size Normal Family Sans
Size Large
EndFont EndFont
End End
@ -253,9 +249,10 @@ Style Subsection
TopSep 1.7 TopSep 1.7
BottomSep 1.1 BottomSep 1.1
Font Font
Family Sans
Series Medium Series Medium
Size Normal Size Large
Shape Italic Shape Slanted
EndFont EndFont
End End
@ -273,26 +270,29 @@ End
Style Title Style Title
TopSep 2 TopSep 2
BottomSep 1.3 BottomSep 1.3
Align Left Align Center
AlignPossible Left AlignPossible Left
Font Font
Family Sans
Series Bold Series Bold
EndFont EndFont
End End
# Author style redefinition # Author style redefinition
Style Author Style Author
Align Left Align Center
AlignPossible Left AlignPossible Center
LabelType No_Label LabelType No_Label
BottomSep 1.5
Font Font
Size Normal Size Large
Series Bold Series Medium
EndFont EndFont
End End
# Date style redefinition # Date style redefinition
Style Date Style Date
LeftMargin MMM
LabelSep "" LabelSep ""
TopSep 1.2 TopSep 1.2
Align Left Align Left
@ -304,18 +304,32 @@ End
# Abstract style redefinition # Abstract style redefinition
Style Abstract Style Abstract
LeftMargin "" Margin First_Dynamic
RightMargin "" LatexType Command
LatexName abstract
InTitle 1
NextNoIndent 1
LeftMargin MMM
RightMargin MMM
ParIndent "" ParIndent ""
TopSep 1.4 ItemSep 0
TopSep 1.2
BottomSep 0.7 BottomSep 0.7
LabelType Top_Environment ParSep 0
Align Block
AlignPossible Block
LabelType static
LabelString " Abstract "
LabelSep M
LabelBottomSep 0
Font Font
Size Normal Size Small
EndFont EndFont
LabelFont LabelFont
Family Sans
Series Bold Series Bold
Size Normal Size Small
EndFont EndFont
End End

134
lib/layouts/aapaper.inc Normal file
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@ -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
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@ -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

42
lib/templates/aa.lyx
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@ -1,12 +1,13 @@
#This file was created by <pit> Mon Nov 24 23:26:21 1997 #LyX 1.1 created this file. For more info see http://www.lyx.org/
#LyX 0.11 (C) 1995-1997 Matthias Ettrich and the LyX Team \lyxformat 218
\lyxformat 2.15
\textclass aa \textclass aa
\language english \language english
\inputencoding auto
\fontscheme times \fontscheme times
\graphics default \graphics default
\paperfontsize default \paperfontsize default
\spacing single \spacing single
\papersize Default
\paperpackage a4 \paperpackage a4
\use_geometry 0 \use_geometry 0
\use_amsmath 0 \use_amsmath 0
@ -15,13 +16,12 @@
\tocdepth 3 \tocdepth 3
\paragraph_separation indent \paragraph_separation indent
\defskip medskip \defskip medskip
\quotes_language english
\quotes_times 2
\papercolumns 2 \papercolumns 2
\papersides 2 \papersides 2
\paperpagestyle default \paperpagestyle default
\layout Thesaurus
Put the Thesaurus codes here
\layout Title \layout Title
This is your Title This is your Title
@ -54,29 +54,45 @@ inst{
\layout Address \layout Address
Here Here
\newline
\latex latex \latex latex
\backslash
email{
\latex default
myaddress
\latex latex
}
\newline
\backslash \backslash
and and
\latex default \latex default
There There
\layout Offprint \newline
Me \latex latex
\layout Email
\backslash
email{
\latex default
youraddress
\latex latex
}
\layout Offprint
Me Me
\layout Date \layout Date
Received / Accepted Received ; Accepted
\layout Abstract \layout Abstract
Short abstract Short abstract
\layout Abstract
\latex latex \latex latex
\newline
\backslash \backslash
keywords{ keywords{
\latex default \latex default