All Figures

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{4820fg1.eps} \end{figure}$ Figure 1: The H I absorption profile detected in J0111+3906. The velocity is in the optical heliocentric convention.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=9cm,clip]{4820fg2a.eps}\par\vspace*{2mm} \includegraphics[width=8.3cm,clip]{4820fg2b.eps} \end{figure}$ Figure 2: a) The H I absorption profile detected in OQ 208 from our new WSRT observations. The velocity is in the optical heliocentric convention. Strong RFI is present in the line profile. b) The two-epoch line profiles of OQ 208 one superimposed to the other; the continuous line represents data from Morganti et al. (2005), while the dotted line represents our new data. c) The residuals obtained after subtracting the two-epoch line profiles.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6.7cm,clip]{4820fg3.ps} \end{figure}$ Figure 3: H I total intensity contours superimposed onto a DSS optical image centered on the radio galaxy J0655+4100. Two nearby galaxies are clearly detected. Contours levels are: 2.35, 3.50, 5.68 and $7.51 \times 10^{20}$ atoms cm^-2.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{4820fg4.eps} \end{figure}$ Figure 4: Absorbed H I column density versus projected linear sizes. The HFP galaxies do not seem to follow the trend found for CSS/GPS sources. The CSS/GPS values have been taken from Pihlström et al. (2003).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{4820fg5.eps} \end{figure}$ Figure 5: Cartoon of a possible orientation of the HFP sources and circumnuclear torus. The toroidal structure is perpendicular to the source axis. The torus model is dependent on the opening angle $\theta$ and the viewing angle $\alpha$ . The scale shown is approximate: the inner radius of the torus and the sizes of the denser clumps are not known.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{4820fg1.eps} \end{figure}$	Figure 1: The H I absorption profile detected in J0111+3906. The velocity is in the optical heliocentric convention.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6.7cm,clip]{4820fg3.ps} \end{figure}$	Figure 3: H I total intensity contours superimposed onto a DSS optical image centered on the radio galaxy J0655+4100. Two nearby galaxies are clearly detected. Contours levels are: 2.35, 3.50, 5.68 and $7.51 \times 10^{20}$ atoms cm^-2.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{4820fg4.eps} \end{figure}$	Figure 4: Absorbed H I column density versus projected linear sizes. The HFP galaxies do not seem to follow the trend found for CSS/GPS sources. The CSS/GPS values have been taken from Pihlström et al. (2003).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{4820fg5.eps} \end{figure}$	Figure 5: Cartoon of a possible orientation of the HFP sources and circumnuclear torus. The toroidal structure is perpendicular to the source axis. The torus model is dependent on the opening angle $\theta$ and the viewing angle $\alpha$ . The scale shown is approximate: the inner radius of the torus and the sizes of the denser clumps are not known.
Open with DEXTER