diff --git a/manuscript.md b/manuscript.md index 6bcae21..d19333c 100644 --- a/manuscript.md +++ b/manuscript.md @@ -113,7 +113,7 @@ notation: \noindent and with the definitions of the \emph{local cooling time\/} - (see Fig. \ref{FigGam}) + (see [@fig:FigGam] Fig. \ref{FigGam}) \begin{equation} \tau_{\mathrm{co}} = \frac{E_{\mathrm{th}}}{L_{r0}} \,, \end{equation} @@ -363,14 +363,14 @@ Lp. & Miejscowość 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:FigVibStab] == Fig. \ref{fig:FigVibStab} for a picture of $S_{\mathrm{vib}}$. Regions of secular instability are listed in Table 1. -![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} +![Vibrational stability equation of state $S_{\mathrm{vib}}(\lg e, \lg \rho)$. $>0$ means vibrational stability.](Figure/icml_numpapers.eps){#fig:FigVibStab width=3.43in height=2.71in}