All Figures

$\begin{figure} \par\includegraphics[width=13.7cm,clip]{f1a_1401.ps}\addtocounter{figure}{-1} \end{figure}$ Figure 1: HI profiles of the 44 detected galaxies observed with the 100-m Effelsberg radio telescope which has a half power beamwidth of 9.3 arcmin at 21-cm. 21 of theses galaxies have been observed for the first time. Profiles are arranged in increasing order of right ascension, starting at the bottom left of this figure (see Table 1). The axes are given in Jansky (Jy) and in heliocentric radial velocity in km s^-1.
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In the text

$\begin{figure} \par\includegraphics[width=13.4cm,clip]{f1b_1401.ps}\end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\includegraphics[width=6.45cm,clip]{f2__1401.ps}\end{figure}$ Figure 2: The relative content of neutral hydrogen $M_{{\rm HI}}$ /L_B of the detected galaxies is plotted versus blue absolute magnitude M_B. The solid line represents the sample of nearby galaxies (KKHM). The range covered by both coordinates is the total range covered by the comparison sample.
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In the text

$\begin{figure} \par\includegraphics[width=6.2cm,clip]{f3__1401.ps}\end{figure}$ Figure 3: The linear diameter A₀ is given versus the absolute blue magnitude of all galaxies of our sample. The solid line represents the sample of nearby galaxies (KKHM). The range covered by both coordinates is the total range covered by the comparison sample.
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In the text

$\begin{figure} \par\includegraphics[width=13.4cm,clip]{f1b_1401.ps}\end{figure}$	Figure 1: continued.
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$\begin{figure} \par\includegraphics[width=6.45cm,clip]{f2__1401.ps}\end{figure}$	Figure 2: The relative content of neutral hydrogen $M_{{\rm HI}}$ /L_B of the detected galaxies is plotted versus blue absolute magnitude M_B. The solid line represents the sample of nearby galaxies (KKHM). The range covered by both coordinates is the total range covered by the comparison sample.
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$\begin{figure} \par\includegraphics[width=6.2cm,clip]{f3__1401.ps}\end{figure}$	Figure 3: The linear diameter A₀ is given versus the absolute blue magnitude of all galaxies of our sample. The solid line represents the sample of nearby galaxies (KKHM). The range covered by both coordinates is the total range covered by the comparison sample.
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