All Figures

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{8142fig1.eps} \end{figure}$ Figure 1: HST/WFPC2 F814W archival image of He 2-10 with an overlaid CO (thick white) contour from Kobulnicky et al. (1995). The thin black lines outline the positions of bubbles observed in H $\alpha$ emission (Méndez et al. 1999). The inset shows the central region at larger scale together with the footprint of our ARGUS observations and regions A and B, as discussed in the text.
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In the text

$\begin{figure} \par\includegraphics[width=8.25cm,clip]{8142fig2.eps} \end{figure}$ Figure 2: Example of two spectra in arbitrary flux units from single fibres with different S/N. Dotted line: original spectrum. Solid line: after subtraction of the Paschen lines.
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In the text

$\begin{figure} \par\includegraphics[width=8cm]{8142fig3.eps} \end{figure}$ Figure 3: Panels showing the field of view of ARGUS, 22 by 14 pixels, corresponding to $11\hbox{$.\!\!^{\prime\prime}$ }4$ $\times$ $7\hbox{$.\!\!^{\prime\prime}$ }3$ . As indicated in Fig. 1, north-east is to the left and north-west at the top of each field of view. Panels a) and b) show the continuum emission near the Ca triplet and the monochromatic emission from [S III] respectively, in arbitrary flux units. Panels c) and d): heliocentric line-of-sight velocity and velocity dispersion from the Ca triplet. Colours for these and the following panels indicate values according to the colour bars below each column. Panels e) and f): velocity and velocity dispersion from [S III]. Panels g) and h): velocity and velocity dispersion from the Paschen lines.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{8142fig1.eps} \end{figure}$	Figure 1: HST/WFPC2 F814W archival image of He 2-10 with an overlaid CO (thick white) contour from Kobulnicky et al. (1995). The thin black lines outline the positions of bubbles observed in H $\alpha$ emission (Méndez et al. 1999). The inset shows the central region at larger scale together with the footprint of our ARGUS observations and regions A and B, as discussed in the text.
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$\begin{figure} \par\includegraphics[width=8.25cm,clip]{8142fig2.eps} \end{figure}$	Figure 2: Example of two spectra in arbitrary flux units from single fibres with different S/N. Dotted line: original spectrum. Solid line: after subtraction of the Paschen lines.
Open with DEXTER