All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{2804fig1.ps} \end{figure}$ Figure 1: Extract of the disentangled component spectra around a blemish in the input spectra. The original result is shifted down by 0.02 relative to the one obtained from improved input spectra. The spectra of V578 Mon B are shifted down 0.09 relative to V578 Mon A.
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In the text

$\begin{figure} \includegraphics[width=8.8cm,clip]{2804fig2.ps} \end{figure}$ Figure 2: Six spectral regions containing temperature-dependent lines and line blends. Each panel shows, from top to bottom: the sharp-lined O9.5 #180 and an artificially blurred version mimicking the rotational broadening in V578 Mon A; the spectra of V578 Mon A and V578 Mon B; and the sharp-lined B1V #201 and an artificially blurred version mimicking the rotational broadening in V578 Mon B. The most important absorbers are identified. The applied vertical shift to the spectra is indicated by dashed lines representing the continuum levels.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{2804fig1.ps} \end{figure}$	Figure 1: Extract of the disentangled component spectra around a blemish in the input spectra. The original result is shifted down by 0.02 relative to the one obtained from improved input spectra. The spectra of V578 Mon B are shifted down 0.09 relative to V578 Mon A.
Open with DEXTER