The HI content of spirals. II. Gas deficiency in cluster galaxies

We derive the atomic hydrogen content for a total of 1900 spirals in the fi elds of 18 nearby clusters. By comparing the H I-deficiency distributions o f the galaxies inside and outside one Abell radius (R-A) of each cluster, w e find that two-thirds of the clusters in our sample show a dearth of neutr al gas in their interiors. Possible connections between the gaseous deficie ncy and the characteristics of both the underlying galaxies and their envir onment are investigated in order to gain insight into the mechanisms respon sible for H I depletion. While we do not find a statistically significant v ariation of the fraction of H I-deficient spirals in a cluster with its glo bal properties, a number of correlations emerge that argue in favor of the interplay between spiral disks and their environment. In the clusters in wh ich neutral gas deficiency is pronounced, we see clear indications that the degree of H I depletion is related to the morphology of the galaxies and n ot to their optical size; early-type and probably dwarf spirals are more ea sily emptied of gas than the intermediate Sbc-Sc types. Gas contents below 1/10, and even 1/100, of the expectation value have been measured, implying that gas removal is very efficient. The radial extent of the region with s ignificant gas ablation can reach up to 2R(A). Within this zone, the propor tion of gas-poor spirals increases continuously toward the cluster center. The wealth of 21 cm data collected for the Virgo region has made it possibl e to study the two-dimensional pattern of H I deficiency in that cluster. T he map of gas deficiency in the Virgo central area points to an scenario in which gas losses result from the interaction of the disks with the inner h ot intracluster gas around M87. We also find evidence that gas-poor spirals in H I-deficient clusters move in orbits more radial than those of the gas -rich objects. The implications of all these results on models of how galax ies interact with their environment are reviewed. Hydrodynamic effects appe ar as the most plausible cause of H I removal.