Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=6.1cm,clip]{Hb231_f1.eps}\end{figure}$ Figure 1: Composite image obtained by superposition of radio images at 43, 22 and 14.9 GHz. Color coding is: 14.9 GHz red, 22.0 GHz green and 43.0 GHz blue.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{Hb231_f2.eps}\hspace*{4mm} \includegraphics[width=6.8cm,clip]{Hb231_f3.eps}\end{figure}$ Figure 2: a) Contour plot of 1.3 cm image. Levels are -3, 3, 4, 5, 6, 7, 8, 10, 12, 15, 20, 25, 30, 40, 45, 50, 60, 70, 80, 90 times 0.09 mJy/beam; b) Contour plot of 0.7 cm image. Levels are -3, 3, 4, 5, 6, 7, 8, 10, 12, 15, 20, 25, 30, 40, 45, 50, 60, 70, 80, 90 times 0.15 mJy/beam.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.15cm,clip]{Hb231_f4.eps}\end{figure}$ Figure 3: Radio spectra of the central object and of the extended nebula. For the compact object, triangles indicate the measurements used in the fit to derive the spectral index. Diamonds indicate extrapolations of such a fit to the lower frequencies. For the extended nebula, the optically thick spectrum (dotted line) and optically thin spectrum (dashed line) of a free-free emitting radio sources are shown for comparison.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6.1cm,clip]{Hb231_f1.eps}\end{figure}$	Figure 1: Composite image obtained by superposition of radio images at 43, 22 and 14.9 GHz. Color coding is: 14.9 GHz red, 22.0 GHz green and 43.0 GHz blue.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{Hb231_f2.eps}\hspace*{4mm} \includegraphics[width=6.8cm,clip]{Hb231_f3.eps}\end{figure}$	Figure 2: a) Contour plot of 1.3 cm image. Levels are -3, 3, 4, 5, 6, 7, 8, 10, 12, 15, 20, 25, 30, 40, 45, 50, 60, 70, 80, 90 times 0.09 mJy/beam; b) Contour plot of 0.7 cm image. Levels are -3, 3, 4, 5, 6, 7, 8, 10, 12, 15, 20, 25, 30, 40, 45, 50, 60, 70, 80, 90 times 0.15 mJy/beam.
Open with DEXTER