#LyX 2.2 created this file. For more info see http://www.lyx.org/
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+\save_transient_properties true
\origin /systemlyxdir/examples/
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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
\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
\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 Separator parbreak
\end_inset
+
\end_layout
\begin_layout Standard
), 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">
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+<features tabularvalignment="middle">
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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
\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
\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
+ gievn 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