Astronomy & Astrophysics

$\begin{figure}\setlength{\unitlength}{0.985cm} \begin{picture} (8.0,23.) \put(-... ...ffset=25 voffset=30 hscale=33 vscale=33 angle=0}} \end{picture} \par\end{figure}$ Figure 1: Gray-scale representation of the ISOPHOT 60 $\mu$ m (top), 70 $\mu$ m (middle), 90 $\mu$ m (bottom) map of NGC 7078 for the first epoch observation; the scale at the bottom applies to all three images. Horizontal and vertical scales are in pixels; pixel size is 45 $^{\prime \prime }$ .
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In the text

$\begin{figure} \setlength{\unitlength}{1cm} \begin{picture} (8.0,4.2) \put(-0.2... ...hoffset=30 voffset=185 hscale=25 vscale=25 angle=270}} \end{picture}\end{figure}$ Figure 2: Colour-corrected ISOPHOT fluxes from central $3\times 3$ pixels of NGC 7078 (filled circles) compared with the stellar contribution (filled triangles). Solid curve is 4200 K blackbody fitted to $U\!BV$ data; broken curve corresponds to fayalite at 50 K. See text for details.
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In the text

$\begin{figure}\setlength{\unitlength}{0.985cm} \begin{picture} (8.0,23.) \put(-... ...ffset=25 voffset=30 hscale=33 vscale=33 angle=0}} \end{picture} \par\end{figure}$	Figure 1: Gray-scale representation of the ISOPHOT 60 $\mu$ m (top), 70 $\mu$ m (middle), 90 $\mu$ m (bottom) map of NGC 7078 for the first epoch observation; the scale at the bottom applies to all three images. Horizontal and vertical scales are in pixels; pixel size is 45 $^{\prime \prime }$ .
Open with DEXTER

$\begin{figure} \setlength{\unitlength}{1cm} \begin{picture} (8.0,4.2) \put(-0.2... ...hoffset=30 voffset=185 hscale=25 vscale=25 angle=270}} \end{picture}\end{figure}$	Figure 2: Colour-corrected ISOPHOT fluxes from central $3\times 3$ pixels of NGC 7078 (filled circles) compared with the stellar contribution (filled triangles). Solid curve is 4200 K blackbody fitted to $U\!BV$ data; broken curve corresponds to fayalite at 50 K. See text for details.
Open with DEXTER