All Figures

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{2535fig1.eps} \end{figure}$ Figure 1: The ${\Sigma -D}$ diagram at a frequency of 1 GHz for 21 M 82 calibrators.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{2535fig2.eps} \end{figure}$ Figure 2: The ${\Sigma -D}$ diagram at a frequency of 1 GHz. The SNRs are represented by: asterisks (LMC), open circles (SMC), filled triangles (M 31), filled dots (M 33), open box (IC 1613), open squares (NGC 300), filled circles (NGC 7793), open triangles (NGC 6946), "x'''s (M 82), crosses (NGC 2146) and open diamonds (NGC 1569).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{2535fig3.eps} \end{figure}$ Figure 3: Sensitivity lines in the ${\Sigma -D}$ plane for radio surveys of 11 nearby galaxies at 1.4 GHz. The sensitivity lines for M 82 and NGC 2146 are at 8.4 GHz and 1.6 GHz, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{2535fig1.eps} \end{figure}$	Figure 1: The ${\Sigma -D}$ diagram at a frequency of 1 GHz for 21 M 82 calibrators.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{2535fig2.eps} \end{figure}$	Figure 2: The ${\Sigma -D}$ diagram at a frequency of 1 GHz. The SNRs are represented by: asterisks (LMC), open circles (SMC), filled triangles (M 31), filled dots (M 33), open box (IC 1613), open squares (NGC 300), filled circles (NGC 7793), open triangles (NGC 6946), "x'''s (M 82), crosses (NGC 2146) and open diamonds (NGC 1569).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{2535fig3.eps} \end{figure}$	Figure 3: Sensitivity lines in the ${\Sigma -D}$ plane for radio surveys of 11 nearby galaxies at 1.4 GHz. The sensitivity lines for M 82 and NGC 2146 are at 8.4 GHz and 1.6 GHz, respectively.
Open with DEXTER