All Figures

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{5992fig1.eps}\end{figure}$ Figure 1: A sample spectrogram belonging to SMC N 88A. The upper panel shows the 2D spectrum and the lower panel a cut through the central row, with relative intensity scale.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{5992fig2a}\vspace*{3mm} \includegraphics[width=9cm,clip]{5992fig2b}\end{figure}$ Figure 2: Excitation (measured by the line ratio [ O III] $\lambda$ $\lambda$ 4959 + 5007/ $\ensuremath {{{\rm H}\beta }}$ ) versus the $\ensuremath {{{\rm H}\beta }}$ luminosity for the SMC and LMC objects. The logarithmic luminosity scale is in units of watts W, 10⁷ erg s^-1 as well as in units of solar bolometric luminosity. The figures are based on the data presented in Tables 3 and 2, respectively. Solid lines: least-square fits for the SMC and LMC objects. Dashed line: least-square fit for the LMC sample, excluding HEBs (filled dots).
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{5992fig1.eps}\end{figure}$	Figure 1: A sample spectrogram belonging to SMC N 88A. The upper panel shows the 2D spectrum and the lower panel a cut through the central row, with relative intensity scale.
Open with DEXTER