All Figures

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{Hk282_fig1.eps} \end{figure}$ Figure 1: Spatial variation of selected physical quantities for the representative model WR123U. The curves labelled $\delta r/r$ and ${\rm d} W /{\rm d} r$ stand for the relative radius perturbations and the differential work, respectively. The dash-dotted curve delineates the scaled spatial variation of the opacity derivative $\kappa_T \equiv (\partial \log \kappa / \partial \log T)_P$ .
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In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{Hk282_fig2.eps} \end{figure}$ Figure 2: Initial growth of photospheric velocity of model WR123U. The dotted line indicates the growth of the amplitude as computed from a linear non-adiabatic analysis. After about 28 days, non-linear saturation forces the model into its final pulsation amplitude.
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In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{Hk282_fig3.eps} \end{figure}$ Figure 3: Light curves in the B and V filter passbands as a function of pulsational phase for the representative model WR123U. The period of the variability is 0.493 d. The V light curve is shifted arbitrarily by 0.2 mag.
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In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{Hk282_fig1.eps} \end{figure}$	Figure 1: Spatial variation of selected physical quantities for the representative model WR123U. The curves labelled $\delta r/r$ and ${\rm d} W /{\rm d} r$ stand for the relative radius perturbations and the differential work, respectively. The dash-dotted curve delineates the scaled spatial variation of the opacity derivative $\kappa_T \equiv (\partial \log \kappa / \partial \log T)_P$ .
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$\begin{figure} \par\includegraphics[width=7.7cm,clip]{Hk282_fig2.eps} \end{figure}$	Figure 2: Initial growth of photospheric velocity of model WR123U. The dotted line indicates the growth of the amplitude as computed from a linear non-adiabatic analysis. After about 28 days, non-linear saturation forces the model into its final pulsation amplitude.
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$\begin{figure} \par\includegraphics[width=7.7cm,clip]{Hk282_fig3.eps} \end{figure}$	Figure 3: Light curves in the B and V filter passbands as a function of pulsational phase for the representative model WR123U. The period of the variability is 0.493 d. The V light curve is shifted arbitrarily by 0.2 mag.
Open with DEXTER