-#LyX 2.2 created this file. For more info see http://www.lyx.org/
-\lyxformat 504
+#LyX 2.3 created this file. For more info see http://www.lyx.org/
+\lyxformat 544
\begin_document
\begin_header
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\index Index
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-This is an example \SpecialCharNoPassThru LyX
- file for articles to be submitted to the Journal
- of Astronomy & Astrophysics (A&A).
- How to install the A&A \SpecialCharNoPassThru LaTeX
- class to your \SpecialCharNoPassThru LaTeX
- system is explained in
-
+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
\family sans
aa.lyx
\family default
- template file that comes with \SpecialCharNoPassThru LyX
+ template file that comes with \SpecialChar LyX
.
\end_layout
\end_layout
\begin_layout Keywords
-giant planet formation \twohyphens
-
+giant planet formation –
\begin_inset Formula $\kappa$
\end_inset
--mechanism \twohyphens
- stability of gas spheres
+-mechanism – stability of gas spheres
\end_layout
\begin_layout Section
\begin_inset CommandInset citation
LatexCommand cite
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
(
\begin_inset CommandInset citation
LatexCommand cite
key "Abernethy2003"
+literal "true"
\end_inset
\begin_inset CommandInset citation
LatexCommand cite
key "Cotton1999"
+literal "true"
\end_inset
\begin_inset CommandInset citation
LatexCommand cite
key "Mena2000"
+literal "true"
\end_inset
\begin_inset CommandInset citation
LatexCommand cite
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.
\begin_inset CommandInset citation
LatexCommand cite
key "Abernethy2003"
+literal "true"
\end_inset
\begin_inset CommandInset citation
LatexCommand cite
key "Abernethy2003"
+literal "true"
\end_inset
).
Using Baker's notation:
-\begin_inset Separator parbreak
-\end_inset
-
\end_layout
\begin_layout Standard
\begin_inset CommandInset citation
LatexCommand cite
key "Abernethy2003"
+literal "true"
\end_inset
\begin_inset CommandInset citation
LatexCommand cite
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 \twohyphens
- or in other words the layer \twohyphens
- 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
\align center
\begin_inset Tabular
<lyxtabular version="3" rows="4" columns="2">
-<features rotate="0" tabularvalignment="middle">
+<features tabularvalignment="middle">
<column alignment="left" valignment="top" width="0pt">
<column alignment="left" valignment="top" width="0pt">
<row>
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
\begin_inset CommandInset citation
LatexCommand cite
key "Abernethy2003"
+literal "true"
\end_inset
\end_layout
\begin_layout Enumerate
-If the constitutive relations \twohyphens
- equations of state and Rosseland mean opacities
- \twohyphens
- 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_inset space ~
\end_inset
-17/2\twohyphens
-1.
+17/2–1.
\end_layout
\begin_layout Standard
Note:
\series default
If you cannot see the bibliography in the output, assure that you have
- gievn the full path to the Bib\SpecialCharNoPassThru TeX
+ given the full path to the Bib\SpecialChar TeX
style file
\family sans
aa.bst
\family default
- that is part of the A&A \SpecialCharNoPassThru LaTeX
+ that is part of the A&A \SpecialChar LaTeX
-package.
\end_layout