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$\begin{figure} \par\includegraphics[width=8cm]{0641f1}\end{figure}$ Figure 1: Opacity $\kappa _{\rm rp}$ of forsterite grains in units of the critical opacity $\kappa _{\rm crit}$ ( $M_{\star}= 1~M_{\odot}$ , $L_{\star}= 7000~L_{\odot}$ ), assuming that 30 percent of Si is condensed into grains; The black contour shows the region where the flux-weighted opacity exceeds the critical opacity, assuming a Planckian flux distribution with $T_{\star }= 2700$ K.
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In the text

$\begin{figure} \par\hspace*{-2mm}\includegraphics[width=7.2cm]{0641f2ab} % \par\vspace*{5mm} \includegraphics[width=7cm]{0641f2c}\end{figure}$ Figure 2: Snapshot of the spatial structure of model B with $n_{\rm gr}/n_{\rm H} = 1$ $\times$ 10^-15: top: velocity, middle: grain radius, bottom: grain temperature (solid) and gas temperature (dashed).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm]{0641f1}\end{figure}$	Figure 1: Opacity $\kappa _{\rm rp}$ of forsterite grains in units of the critical opacity $\kappa _{\rm crit}$ ( $M_{\star}= 1~M_{\odot}$ , $L_{\star}= 7000~L_{\odot}$ ), assuming that 30 percent of Si is condensed into grains; The black contour shows the region where the flux-weighted opacity exceeds the critical opacity, assuming a Planckian flux distribution with $T_{\star }= 2700$ K.
Open with DEXTER

$\begin{figure} \par\hspace{-2mm}\includegraphics[width=7.2cm]{0641f2ab} % \par\vspace{5mm} \includegraphics[width=7cm]{0641f2c}\end{figure}$	Figure 2: Snapshot of the spatial structure of model B with $n_{\rm gr}/n_{\rm H} = 1$ $\times$ 10^-15: top: velocity, middle: grain radius, bottom: grain temperature (solid) and gas temperature (dashed).
Open with DEXTER