Fig. 12
The number ratio of HI-rich LTGs over all LTGs as a function of the velocity dispersion (panel a)) and of the local density (panel b)) of 7 groups (small dots) and their average (triangle), the Coma cluster (square) and the field (large dot). The last point has been plotted at 100σ = km s-1 to represent that, even in the field, galaxies are subject to random motions.
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