**Table 2:** Galaxy gas properties.
$\begin{table} \begin{displaymath} \begin{array}{lccccccccc} \hline\hline\noali... ... 95 & 0.6 & 38 & 1.6 & 10.7\\ \hline \end{array} \end{displaymath}\end{table}$
^a Cayatte et al. (1994); ^b Oosterloo & van Gorkom (2005); ^c Crowl et al. (2005); ^d We took the HI deficiency of NGC 4579 which has about the same B and H band magnitudes and morphological type. As NGC 4438, it also shows a highly truncated gas disk with a very small amount of H I; ^e CO gas mass from Vollmer et al. (2006); ^f from this paper; ^g Kenney et al. (2004); ^h Vollmer & Huchtmeier (2003); ⁱ based on the low mass and low surface brightness extraplanar H I; ^j Vollmer et al. (2005); ^k Vollmer et al., in prep.; ^l Vollmer et al. (2006); ^m Vollmer et al. (2004a).

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