next previous
Up: Understanding A-type supergiants


6 Figure 1 to 3 in electronic form only

 
\begin{figure}
\includegraphics []{figure1a.ps}
\end{figure} Figure 1: Spectral atlas of stars with visible spectra only. The laboratory wavelengths of the lines are marked by a vertical dashed line

 
\begin{figure}
\includegraphics []{figure1b.ps}
\end{figure} Figure 1: continued

 
\begin{figure}
\includegraphics []{figure1c.ps}
\end{figure} Figure 1: continued

 
\begin{figure}
\includegraphics []{hd2928.ps}
\end{figure} Figure 2: Spectral atlas of stars with visible and ultraviolet spectra. As in Fig. 1 the laboratory wavelengths are marked with dashed lines

 
\begin{figure}
\includegraphics []{hd3940.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd5776.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd12953.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd13476.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd13744.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd14433.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd14489.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd14535.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd15316.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd16778.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd17378.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd20041.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd21389.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd46300.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd59612.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd87737.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd92207.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd100198.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd100826.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd102878.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd103516.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd104035.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd104111.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd161912.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd197345.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd207260.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd207673.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd210221.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd211971.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd212593.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd213470.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd223385.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{hd223960.ps}
\end{figure} Figure 2: continued

 
\begin{figure}
\includegraphics []{figure3a.ps}
\end{figure} Figure 3: Some examples of spectra variability

 
\begin{figure}
\includegraphics []{figure3b.ps}
\end{figure} Figure 3: continued

 
\begin{figure}
\includegraphics []{figure3c.ps}
\end{figure} Figure 3: continued

 
\begin{figure}
\includegraphics []{figure3d.ps}
\end{figure} Figure 3: continued

 
\begin{figure}
\includegraphics [angle=90]{figure3e.ps}
\end{figure} Figure 3: continued

next previous
Up: Understanding A-type supergiants

Copyright The European Southern Observatory (ESO)