-#LyX 2.0 created this file. For more info see http://www.lyx.org/
-\lyxformat 413
+#LyX 2.3 created this file. For more info see http://www.lyx.org/
+\lyxformat 544
\begin_document
\begin_header
+\save_transient_properties true
+\origin /systemlyxdir/examples/
\textclass aa
-\begin_preamble
-\usepackage{graphicx}
-%
-\end_preamble
-\options traditabstract
-\use_default_options false
+\use_default_options true
\maintain_unincluded_children false
\language english
\language_package default
\inputencoding auto
\fontencoding global
-\font_roman default
-\font_sans default
-\font_typewriter default
+\font_roman "default" "default"
+\font_sans "default" "default"
+\font_typewriter "default" "default"
+\font_math "auto" "auto"
\font_default_family default
\use_non_tex_fonts false
\font_sc false
\font_osf false
-\font_sf_scale 100
-\font_tt_scale 100
-
+\font_sf_scale 100 100
+\font_tt_scale 100 100
+\use_microtype false
+\use_dash_ligatures false
\graphics default
\default_output_format default
\output_sync 0
-\bibtex_command default
+\bibtex_command bibtex
\index_command default
\paperfontsize default
\spacing single
\use_hyperref false
\papersize default
\use_geometry false
-\use_amsmath 0
-\use_esint 0
-\use_mhchem 1
-\use_mathdots 1
-\cite_engine basic
+\use_package amsmath 1
+\use_package amssymb 1
+\use_package cancel 1
+\use_package esint 1
+\use_package mathdots 1
+\use_package mathtools 1
+\use_package mhchem 1
+\use_package stackrel 1
+\use_package stmaryrd 1
+\use_package undertilde 1
+\cite_engine natbib
+\cite_engine_type authoryear
+\biblio_style plain
\use_bibtopic false
\use_indices false
\paperorientation portrait
\suppress_date false
+\justification true
\use_refstyle 0
+\use_minted 0
\index Index
\shortcut idx
\color #008000
\tocdepth 3
\paragraph_separation indent
\paragraph_indentation default
-\quotes_language english
+\is_math_indent 0
+\math_numbering_side default
+\quotes_style english
+\dynamic_quotes 0
\papercolumns 2
\papersides 2
\paperpagestyle default
\begin_body
-\begin_layout Standard
+\begin_layout Title
\begin_inset Note Note
status open
\begin_layout Plain Layout
-This is an example LyX file for articles to be submitted to the Journal
- of Astronomy & Astrophysicssing (A&A).
- How to install the A&A LaTeX class to your LaTeX system is explained in
-
+
+\family roman
+\series medium
+\size normal
+This is an example \SpecialChar LyX
+ file for articles to be submitted to the Journal of
+ Astronomy & Astrophysics (A&A).
+ How to install the A&A \SpecialChar LaTeX
+ class to your \SpecialChar LaTeX
+ system is explained in
\begin_inset Flex URL
status open
\begin_layout Plain Layout
-http://wiki.lyx.org/Layouts/Astronomy-Astrophysics
+https://wiki.lyx.org/Layouts/Astronomy-Astrophysics
\end_layout
\end_inset
.
-\end_layout
-
+\begin_inset Newline newline
\end_inset
+Depending on the submission state and the abstract layout, you need to use
+ different document class options that are listed in the aa manual.
+\family default
-\end_layout
+\begin_inset Newline newline
+\end_inset
-\begin_layout Standard
-\begin_inset Note Note
-status open
-\begin_layout Plain Layout
-Depending on the submission state and the abstract layout, you need to use
- different document class options that are listed in the aa manual
-\family sans
-aadoc.pdf
-\family default
-.
+\family roman
+\series default
+Note:
+\series medium
+ If you use accented characters in your document, you must use the predefined
+ document class option
+\series default
+latin9
+\series medium
+ in the document settings.
\end_layout
\end_inset
Received September 15, 1996; accepted March 16, 1997
\end_layout
-\begin_layout Abstract
-To investigate the physical nature of the `nuc\SpecialChar \-
+\begin_layout Abstract (unstructured)
+To investigate the physical nature of the `nuc\SpecialChar softhyphen
leated instability' of proto
giant planets, the stability of layers in static, radiative gas spheres
is analysed on the basis of Baker's standard one-zone model.
\family sans
aa.lyx
\family default
- template file that comes with LyX.
+ template file that comes with \SpecialChar LyX
+.
\end_layout
\end_inset
\end_layout
\begin_layout Keywords
-giant planet formation --
+giant planet formation –
\begin_inset Formula $\kappa$
\end_inset
--mechanism -- stability of gas spheres
+-mechanism – stability of gas spheres
\end_layout
\begin_layout Section
Mizuno (
\begin_inset CommandInset citation
LatexCommand cite
-key "mizuno"
+key "Eisenstein2005"
+literal "true"
\end_inset
) determined the critical mass of the core to be about
-\begin_inset Formula $12\, M_{\oplus}$
+\begin_inset Formula $12\,M_{\oplus}$
\end_inset
(
is investigated on the basis of Baker's (
\begin_inset CommandInset citation
LatexCommand cite
-key "baker"
+key "Abernethy2003"
+literal "true"
\end_inset
protostellar cores explode (Tscharnuter
\begin_inset CommandInset citation
LatexCommand cite
-key "tscharnuter"
+key "Cotton1999"
+literal "true"
\end_inset
, Balluch
\begin_inset CommandInset citation
LatexCommand cite
-key "balluch"
+key "Mena2000"
+literal "true"
\end_inset
status open
\begin_layout Plain Layout
-\begin_inset Caption
+\begin_inset Caption Standard
\begin_layout Plain Layout
\begin_inset CommandInset label
In this section the one-zone model of Baker (
\begin_inset CommandInset citation
LatexCommand cite
-key "baker"
+key "Abernethy2003"
+literal "true"
\end_inset
-), originally used to study the Cepheı̈d pulsation mechanism, will be briefly
+), originally used to study the Cepheïd pulsation mechanism, will be briefly
reviewed.
The resulting stability criteria will be rewritten in terms of local state
variables, local timescales and constitutive relations.
Baker (
\begin_inset CommandInset citation
LatexCommand cite
-key "baker"
+key "Abernethy2003"
+literal "true"
\end_inset
c) in Baker
\begin_inset CommandInset citation
LatexCommand cite
-key "baker"
+key "Abernethy2003"
+literal "true"
\end_inset
For a physical discussion of the stability criteria see Baker (
\begin_inset CommandInset citation
LatexCommand cite
-key "baker"
+key "Abernethy2003"
+literal "true"
\end_inset
) or Cox (
\begin_inset CommandInset citation
LatexCommand cite
-key "cox"
+key "Parkin2005"
+literal "true"
\end_inset
), are specified (in practice by specifying a chemical composition) the
one-zone stability can be inferred if the thermodynamic state is specified.
- The zone -- or in other words the layer -- will be stable or unstable in
+ The zone – or in other words the layer – will be stable or unstable in
whatever object it is imbedded as long as it satisfies the one-zone-model
assumptions.
Only the specific growth rates (depending upon the time scales) will be
status open
\begin_layout Plain Layout
-\begin_inset Caption
+\begin_inset Caption Standard
\begin_layout Plain Layout
\begin_inset CommandInset label
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
These depend only on the unperturbed thermodynamical state of the layer.
Therefore the above relations define the one-zone-stability equations of
state
-\begin_inset Formula $S_{\mathrm{dyn}},\, S_{\mathrm{sec}}$
+\begin_inset Formula $S_{\mathrm{dyn}},\,S_{\mathrm{sec}}$
\end_inset
and
status open
\begin_layout Plain Layout
-\begin_inset Caption
+\begin_inset Caption Standard
\begin_layout Plain Layout
\begin_inset CommandInset label
as described by Baker's (
\begin_inset CommandInset citation
LatexCommand cite
-key "baker"
+key "Abernethy2003"
+literal "true"
\end_inset
\end_layout
\begin_layout Enumerate
-If the constitutive relations -- equations of state and Rosseland mean opacities
- -- are specified, the stability equations of state can be evaluated without
+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.
\end_layout
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 Cepheı̈d pulsations.
+y than the second He ionization zone that drives the Cepheïd pulsations.
\end_layout
\begin_layout Acknowledgement
Part of this work was supported by the German
\emph on
-Deut\SpecialChar \-
-sche For\SpecialChar \-
-schungs\SpecialChar \-
-ge\SpecialChar \-
-mein\SpecialChar \-
+Deut\SpecialChar softhyphen
+sche For\SpecialChar softhyphen
+schungs\SpecialChar softhyphen
+ge\SpecialChar softhyphen
+mein\SpecialChar softhyphen
schaft, DFG
\emph default
project number Ts
\begin_inset space ~
\end_inset
-17/2--1.
+17/2–1.
\end_layout
\begin_layout Standard
+\begin_inset CommandInset bibtex
+LatexCommand bibtex
+btprint "btPrintAll"
+bibfiles "biblioExample"
+options "aa"
+
+\end_inset
+
+
\begin_inset Note Note
status open
\begin_layout Plain Layout
-You can alternatively use BibTeX.
- You must then use the BibTeX style
+
+\series bold
+Note:
+\series default
+ If you cannot see the bibliography in the output, assure that you have
+ given the full path to the Bib\SpecialChar TeX
+ style file
\family sans
aa.bst
\family default
- that is part of the A&A LaTeX-package.
+ that is part of the A&A \SpecialChar LaTeX
+-package.
\end_layout
\end_inset
\end_layout
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1966"
-key "baker"
-
-\end_inset
-
- Baker, N.
- 1966, in Stellar Evolution, ed.
-\begin_inset space \space{}
-\end_inset
-
-R.
- F.
- Stein,& A.
- G.
- W.
- Cameron (Plenum, New York) 333
-\end_layout
-
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1988"
-key "balluch"
-
-\end_inset
-
- Balluch, M.
- 1988, A&A, 200, 58
-\end_layout
-
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1980"
-key "cox"
-
-\end_inset
-
- Cox, J.
- P.
- 1980, Theory of Stellar Pulsation (Princeton University Press, Princeton)
- 165
-\end_layout
-
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1969"
-key "cox69"
-
-\end_inset
-
- Cox, A.
- N.,& Stewart, J.
- N.
- 1969, Academia Nauk, Scientific Information 15, 1
-\end_layout
-
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1980"
-key "mizuno"
-
-\end_inset
-
- Mizuno H.
- 1980, Prog.
- Theor.
- Phys., 64, 544
-\end_layout
-
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1987"
-key "tscharnuter"
-
-\end_inset
-
- Tscharnuter W.
- M.
- 1987, A&A, 188, 55
-\end_layout
-
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1992"
-key "terlevich"
-
-\end_inset
-
- Terlevich, R.
- 1992, in ASP Conf.
- Ser.
- 31, Relationships between Active Galactic Nuclei and Starburst Galaxies,
- ed.
- A.
- V.
- Filippenko, 13
-\end_layout
-
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1980a"
-key "yorke80a"
-
-\end_inset
-
- Yorke, H.
- W.
- 1980a, A&A, 86, 286
-\end_layout
-
-\begin_layout Bibliography
-\labelwidthstring References
-\begin_inset CommandInset bibitem
-LatexCommand bibitem
-label "1997"
-key "zheng"
-
-\end_inset
-
-Zheng, W., Davidsen, A.
- F., Tytler, D.
- & Kriss, G.
- A.
- 1997, preprint
-\end_layout
-
\end_body
\end_document
projects / lyx.git / blobdiff