Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4699F1.eps} \end{figure}$ Figure 1: Ratio of the total ¹²CO velocity width to the H I velocity width at 1% of the maximum power versus the projected beam size in units of the optical radius. All ¹²CO detections (i.e. both transitions and both telescopes) are displayed. The dashed line denotes equality.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4699F2.eps} \end{figure}$ Figure 2: Fractional ¹²CO(2-1) line contribution to the 1300 $\mu$ m continuum emission versus the projected beam size in units of the optical radius. Vertical bars mark the rms of the individual values. Open symbols denote upper or lower limits.
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In the text

$\begin{figure} \par\includegraphics[width=17cm,clip]{H4699F3.eps} \end{figure}$ Figure 3: ¹²CO (1-0) and (2-1) spectra from MRT for NGC 145, NGC 178, NGC 959 and IC 292. The full version of Fig. 3 is available at http://www.edpsciences.org.
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In the text

$\begin{figure} \par\includegraphics[width=17cm,clip]{H4699F4.eps} \end{figure}$ Figure 4: ¹²CO (1-0) and (2-1) spectra from SEST for NGC 145, NGC 178, DDO 36 and UGCA 103. The full version of Fig. 4 is available at http://www.edpsciences.org.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4699F1.eps} \end{figure}$	Figure 1: Ratio of the total ¹²CO velocity width to the H I velocity width at 1% of the maximum power versus the projected beam size in units of the optical radius. All ¹²CO detections (i.e. both transitions and both telescopes) are displayed. The dashed line denotes equality.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4699F2.eps} \end{figure}$	Figure 2: Fractional ¹²CO(2-1) line contribution to the 1300 $\mu$ m continuum emission versus the projected beam size in units of the optical radius. Vertical bars mark the rms of the individual values. Open symbols denote upper or lower limits.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{H4699F3.eps} \end{figure}$	Figure 3: ¹²CO (1-0) and (2-1) spectra from MRT for NGC 145, NGC 178, NGC 959 and IC 292. The full version of Fig. 3 is available at http://www.edpsciences.org.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{H4699F4.eps} \end{figure}$	Figure 4: ¹²CO (1-0) and (2-1) spectra from SEST for NGC 145, NGC 178, DDO 36 and UGCA 103. The full version of Fig. 4 is available at http://www.edpsciences.org.
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{H4699F3A.eps} \end{figure}$	Figure 3: continued.
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{H4699F4A.eps} \end{figure}$	Figure 4: continued.
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