Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=13.3cm,clip]{1064fig1.eps}\end{figure}$ Figure 1: Continuum image (grey scale and thin contours; negative contour in light grey) of 4C 12.50 with superimposed the total intensity of the H I absorption (thick contours). The absorption profiles at the two sides of the H I cloud are also shown. The position of the radio core as derived by Stanghellini et al. (1997) and confirmed by Lister et al. (2003) is also indicated. The contour levels for the continuum image are: -5, 5 mJy beam^-1 to 800 mJy beam^-1 in steps of factor 1.5. The contour levels for the total intensity of the H I absorption are -2.5, -2.0, -1.5, -1.0, -0.5 Jy beam^-1 km s^-1.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{1064fig2.ps}\end{figure}$ Figure 2: Comparison between the WSRT profile (black) and the VLBI profile integrated over the H I absorption cloud (dashed).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{1064fig2.ps}\end{figure}$	Figure 2: Comparison between the WSRT profile (black) and the VLBI profile integrated over the H I absorption cloud (dashed).
Open with DEXTER