Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{aa3357f1.ps} \end{figure}$ Figure 1: The logarithm of the number of C stars versus the total absolute V-magnitude of the parent galaxy. The line represents the least-square fit to the points. Filled dots are galaxies with no current star formation.
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In the text

$\begin{figure} \par\includegraphics[width=8.1cm,clip]{aa3357f2.ps} \end{figure}$ Figure 2: Two examples of different C star colour distributions. The left panels represents M 31 and the right ones corresponds to NGC 3109.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{aa3357f3.ps} \end{figure}$ Figure 3: The mean absolute I-magnitude of C stars is plotted versus the total absolute V-magnitude of the parent galaxy. Black dots mark galaxies with over than 100 C stars. The line represents the average magnitude of the black dots.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{aa3357f4.ps} \end{figure}$ Figure 4: The mean absolute I-magnitude of C stars versus the adopted metallicity of the parent galaxy (as listed in Table 1). The straight line represents the least-square fit excluding And II and VII.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{aa3357f1.ps} \end{figure}$	Figure 1: The logarithm of the number of C stars versus the total absolute V-magnitude of the parent galaxy. The line represents the least-square fit to the points. Filled dots are galaxies with no current star formation.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.1cm,clip]{aa3357f2.ps} \end{figure}$	Figure 2: Two examples of different C star colour distributions. The left panels represents M 31 and the right ones corresponds to NGC 3109.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{aa3357f3.ps} \end{figure}$	Figure 3: The mean absolute I-magnitude of C stars is plotted versus the total absolute V-magnitude of the parent galaxy. Black dots mark galaxies with over than 100 C stars. The line represents the average magnitude of the black dots.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{aa3357f4.ps} \end{figure}$	Figure 4: The mean absolute I-magnitude of C stars versus the adopted metallicity of the parent galaxy (as listed in Table 1). The straight line represents the least-square fit excluding And II and VII.
Open with DEXTER