diff --git a/lib/ChangeLog b/lib/ChangeLog index 0b840df4d2..20c156e02d 100644 --- a/lib/ChangeLog +++ b/lib/ChangeLog @@ -1,3 +1,17 @@ +2001-06-12 Peter Suetterlin + + * 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 * doc/LaTeXConfig.lyx.in: @@ -24,12 +38,12 @@ 2001-05-22 Adrien Rebollo - * lib/kbd/european.kmap: - * lib/kbd/francais.kmap: - * lib/kbd/iso8859-15.cdef: + * kbd/european.kmap: + * kbd/francais.kmap: + * kbd/iso8859-15.cdef: * encodings: add iso8859-15 support. - * lib/kbd/iso8859-1.cdef: cleanup + * kbd/iso8859-1.cdef: cleanup 2001-05-22 Peter Suetterlin diff --git a/lib/doc/LaTeXConfig.lyx.in b/lib/doc/LaTeXConfig.lyx.in index 0485ffa879..870d0c58b2 100644 --- a/lib/doc/LaTeXConfig.lyx.in +++ b/lib/doc/LaTeXConfig.lyx.in @@ -360,16 +360,16 @@ Additional document classes aa \layout Description -Found: @chk_aapaper@ +Found: @chk_aa@ \layout Description -CTAN: N/A (available from Springer's ftp site +CTAN: N/A (available from ftp site \family typewriter - ftp.springer.de + ftp.edpsciences.org \family default in directory \family typewriter -/pub/tex/latex/aa +/pub/aa/ \family default ) \layout Description @@ -378,16 +378,13 @@ Notes: The document class \family sans aa \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 Astronomy and Astrophysics \emph default - and the accompanying -\emph on -Supplement Series -\emph default -published by Springer -Verlag. +published by EDP Sciences. \layout Subsection aastex diff --git a/lib/examples/aa_head.lyx b/lib/examples/aa_head.lyx deleted file mode 100644 index fd4b0bb8d5..0000000000 --- a/lib/examples/aa_head.lyx +++ /dev/null @@ -1,153 +0,0 @@ -#This file was created by 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 diff --git a/lib/examples/aa_paper.lyx b/lib/examples/aa_sample.lyx similarity index 69% rename from lib/examples/aa_paper.lyx rename to lib/examples/aa_sample.lyx index fc9a688033..db4b6d389a 100644 --- a/lib/examples/aa_paper.lyx +++ b/lib/examples/aa_sample.lyx @@ -1,8 +1,12 @@ #LyX 1.1 created this file. For more info see http://www.lyx.org/ \lyxformat 218 \textclass aa +\begin_preamble +\usepackage{graphicx} +% +\end_preamble \language english -\inputencoding latin1 +\inputencoding auto \fontscheme default \graphics default \paperfontsize default @@ -22,9 +26,6 @@ \papersides 2 \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 Hydrodynamics of giant planet formation @@ -39,21 +40,68 @@ I. \layout Author G. - Wuchterl -\layout Address + Wuchterl +\latex latex -Institute for Astronomy (IfA), University of Vienna, Türkenschanzstrasse - 17, A-1180 Vienna +\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 + \layout Offprint G. Wuchterl -\layout Email +\layout Address -wuchterl@amok.ast.univie.ac.at +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 + \layout Date -Received September 15, 1996 / Accepted March 16, 1997 +Received September 15, 1996; accepted March 16, 1997 \layout Abstract To investigate the physical nature of the `nuc\SpecialChar \- @@ -74,9 +122,7 @@ leated instability' of proto opacities and the local thermodynamic state in the layer. Stability and instability can therefore be expressed in the form of stability 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 \begin_inset Formula \( -14\leq \lg \rho /[\mathrm{g}\, \mathrm{cm}^{-3}]\leq 0 \) \end_inset @@ -103,7 +149,7 @@ The stability equations of state are calculated for solar composition and . Regions of instability in the -\begin_inset Formula \( (\rho \, e) \) +\begin_inset Formula \( (\rho ,e) \) \end_inset -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 -mechanism is widespread under `cool' conditions. -\layout Abstract - - \latex latex +\newline + \backslash -keywords{ +keywords{giant planet formation -- +\backslash +( +\backslash +kappa +\backslash +)-mechanism -- stability of gas spheres } \latex default -giant planet formation -- -\begin_inset Formula \( \kappa \) -\end_inset - --mechanism -- stability of gas spheres -\latex latex -} + \layout Section Introduction @@ -137,7 +182,12 @@ Introduction In the \emph on nucleated instability +\latex latex + +\backslash +/{} \emph default +\latex default (also called core instability) hypothesis of giant planet formation, a critical mass for static core envelope protoplanets has been found. Mizuno ( @@ -171,37 +221,12 @@ Although no hydrodynamical study has been available many workers conjectured \end_inset ) 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 Phenomena similar to the ones described above for giant planet formation have been found in hydrodynamical models concerning star formation where protostellar cores explode (Tscharnuter -\begin_inset LatexCommand \cite{tscarnuter} +\begin_inset LatexCommand \cite{tscharnuter} \end_inset @@ -220,21 +245,10 @@ Baker's standard one-zone model \layout Standard \begin_float wide-fig -\layout Standard - - -\latex latex - -\backslash -rule{0.4pt}{4cm} -\hfill - -\backslash -parbox[b]{55mm}{ \layout Caption Adiabatic exponent -\begin_inset Formula \( \Gamma \) +\begin_inset Formula \( \Gamma _{1} \) \end_inset . @@ -242,7 +256,7 @@ Adiabatic exponent \begin_inset Formula \( \Gamma _{1} \) \end_inset -is plotted as a function of + is plotted as a function of \begin_inset Formula \( \lg \) \end_inset @@ -259,20 +273,22 @@ is plotted as a function of \end_inset +\layout Standard + + \begin_inset LatexCommand \label{FigGam} \end_inset -\latex latex -} \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} \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. @@ -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, +thermal equilibrium, \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 @@ -315,53 +337,60 @@ c) in Baker \end_inset -]. +). Using Baker's notation: +\layout Standard +\align left + \begin_inset Formula \begin{eqnarray*} -M_{\mathrm{r}} & & \mathrm{mass}\, \mathrm{internal}\, \mathrm{to}\, \mathrm{the}\, \mathrm{radius}\, r\\ -m & & \mathrm{mass}\, \mathrm{of}\, \mathrm{the}\, \mathrm{zone}\\ -r_{0} & & \mathrm{unperturbed}\, \mathrm{zone}\, \mathrm{radius}\\ -\rho _{0} & & \mathrm{unperturbed}\, \mathrm{density}\, \mathrm{in}\, \mathrm{the}\, \mathrm{zone}\\ -T_{0} & & \mathrm{unperturbed}\, \mathrm{temperature}\, \mathrm{in}\, \mathrm{the}\, \mathrm{zone}\\ -L_{r0} & & \mathrm{unperturbed}\, \mathrm{luminosity}\\ -E_{\mathrm{th}} & & \mathrm{thermal}\, \mathrm{energy}\, \mathrm{of}\, \mathrm{the}\, \mathrm{zone} +M_{r} & & \textrm{mass internal to the radius }r\\ +m & & \textrm{mass of the zone}\\ +r_{0} & & \textrm{unperturbed zone radius}\\ +\rho _{0} & & \textrm{unperturbed density in the zone}\\ +T_{0} & & \textrm{unperturbed temperature in the zone}\\ +L_{r0} & & \textrm{unperturbed luminosity}\\ +E_{\textrm{th}} & & \textrm{thermal energy of the zone} \end{eqnarray*} \end_inset + +\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 - + \begin_inset Text @@ -546,16 +577,20 @@ Opacity sources Source \end_inset - + \begin_inset Text \layout Standard -T/[K] + +\begin_inset Formula \( T/[\textrm{K}] \) +\end_inset + + \end_inset - + \begin_inset Text @@ -564,13 +599,13 @@ T/[K] Yorke 1979, Yorke 1980a \end_inset - + \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 - + \begin_inset Text \layout Standard @@ -608,7 +643,7 @@ Kr Cox & Stewart 1969 \end_inset - + \begin_inset Text \layout Standard @@ -617,7 +652,7 @@ Cox & Stewart 1969 \begin_inset Formula \( 5000\leq \) \end_inset - + \end_inset @@ -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 diff --git a/lib/layouts/aa.layout b/lib/layouts/aa.layout index 622cd34e17..1ed0532454 100644 --- a/lib/layouts/aa.layout +++ b/lib/layouts/aa.layout @@ -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 diff --git a/lib/layouts/aapaper.inc b/lib/layouts/aapaper.inc new file mode 100644 index 0000000000..eb29dd15b4 --- /dev/null +++ b/lib/layouts/aapaper.inc @@ -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 + +# 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 + + + diff --git a/lib/layouts/aapaper.layout b/lib/layouts/aapaper.layout new file mode 100644 index 0000000000..8c0f94ffec --- /dev/null +++ b/lib/layouts/aapaper.layout @@ -0,0 +1,201 @@ +#% Do not delete the line below; configure depends on this +# \DeclareLaTeXClass[aa]{article (A&A V4)} +# +# Author: Peter Sütterlin + +# 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 + diff --git a/lib/templates/aa.lyx b/lib/templates/aa.lyx index 1645897db3..e68e4c0f08 100644 --- a/lib/templates/aa.lyx +++ b/lib/templates/aa.lyx @@ -1,12 +1,13 @@ -#This file was created by 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