All Figures

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1a.ps} \end{figure}$ Figure 1: Grey scale images and isophotal maps of the HI-detected galaxy systems from POSS-II (F-band). The contour levels are in arbitrary units. The lowest contour corresponds to the 3 $\sigma$ level of the local background. The scale interval was chosen in order to best illustrate both the inner and outer structure of the galaxies.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1b.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1c.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1d.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1e.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1f.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1g.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1h.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1i.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1j.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1k.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1l.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1m.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1n.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1o.ps} \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[width=14cm,clip]{10734f2.eps} \end{figure}$ Figure 2: HI profiles of the 30 SBS galaxies detected in the present Effelsberg observations, with a pencil beam of half-power width of 9.3 arcmin at 21-cm. The HI profiles are arranged in an increasing order of right ascension, starting at the bottom left corner (see Table 1). The axes show flux density in Jansky (Jy) and the heliocentric radial velocity in km s^-1.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1a.ps} \end{figure}$	Figure 1: Grey scale images and isophotal maps of the HI-detected galaxy systems from POSS-II (F-band). The contour levels are in arbitrary units. The lowest contour corresponds to the 3 $\sigma$ level of the local background. The scale interval was chosen in order to best illustrate both the inner and outer structure of the galaxies.
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$\begin{figure} \par\includegraphics[angle=90,width=10cm,clip]{10734f1b.ps} \end{figure}$	Figure 1: continued.
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$\begin{figure} \par\includegraphics[width=14cm,clip]{10734f2.eps} \end{figure}$	Figure 2: HI profiles of the 30 SBS galaxies detected in the present Effelsberg observations, with a pencil beam of half-power width of 9.3 arcmin at 21-cm. The HI profiles are arranged in an increasing order of right ascension, starting at the bottom left corner (see Table 1). The axes show flux density in Jansky (Jy) and the heliocentric radial velocity in km s^-1.
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