clearer... tinggal table, numlist, dan formula

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@@ -94,8 +94,14 @@ acknowledgements:
 
 # Baker's standard one-zone model
 
+
+
+<!-- we need figure* for make it full screen, so it must be in latex code as follows
+-->
+
 \begin{figure*}
 \centering
+\includegraphics{Figure/icml_numpapers.eps}
 \caption{Adiabatic exponent $\Gamma_1$.
             $\Gamma_1$ is plotted as a function of
             $\lg$ internal energy $\mathrm{[erg\,g^{-1}]}$ and $\lg$
@@ -104,7 +110,7 @@ acknowledgements:
  \end{figure*}
 
 In this section the one-zone model of \citet{DudaHart2nd},
-   originally used to study the Cephe{\"{\i}}d pulsation mechanism, will
+originally used to study the Cephe\text{\"{\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.
@@ -112,11 +118,11 @@ acknowledgements:
 \citet{DudaHart2nd} investigates the stability of thin layers in
 self-gravitating,
 spherical gas clouds with the following properties:
-   \begin{itemize}
-      \item hydrostatic equilibrium,
-      \item thermal equilibrium,
-      \item energy transport by grey radiation diffusion.
-   \end{itemize}
+
+* hydrostatic equilibrium,
+* thermal equilibrium,
+* energy transport by grey radiation diffusion.
+
 For the one-zone-model Baker obtains necessary conditions
 for dynamical, secular and vibrational (or pulsational)
 stability (Eqs.\ (34a,\,b,\,c) in Baker \citeyear{DudaHart2nd}). Using Baker's
@@ -124,7 +130,7 @@ acknowledgements:
 
 \noindent
    and with the definitions of the \emph{local cooling time\/}
-   (see Fig.~\ref{FigGam})
+   (see Fig. \ref{FigGam})
    \begin{equation}
       \tau_{\mathrm{co}} = \frac{E_{\mathrm{th}}}{L_{r0}} \,,
    \end{equation}
@@ -222,7 +228,7 @@ acknowledgements:
    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~\ref{KapSou}), are specified (in practice
+   and opacities (see Table \ref{KapSou}), 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
@@ -302,10 +308,16 @@ acknowledgements:
    thermodynamical state of the layer. Therefore the above relations
    define the one-zone-stability equations of state
    $S_{\mathrm{dyn}},\,S_{\mathrm{sec}}$
-   and $S_{\mathrm{vib}}$. See Fig.~\ref{FigVibStab} for a picture of
+   and $S_{\mathrm{vib}}$. See Fig. \ref{FigVibStab} for a picture of
    $S_{\mathrm{vib}}$. Regions of secular instability are
-   listed in Table~1.
+   listed in Table 1.
+
+<!-- calculate height and width of picture manually in inch, using evince -> Properties
+create label for \ref{FigVibStab} using #FigVibStab
+-->
+![Vibrational stability equation of state $S_{\mathrm{vib}}(\lg e, \lg \rho)$. $>0$ means vibrational stability.](Figure/icml_numpapers.eps){#FigVibStab width=3.43in height=2.71in}
 
+<!--
    \begin{figure}
    \centering
       \caption{Vibrational stability equation of state
@@ -314,6 +326,7 @@ acknowledgements:
               }
          \label{FigVibStab}
    \end{figure}
+-->
 
 # Conclusions
 

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