Spiral Galaxies in MKW/AWM Clusters

Details Spiral Galaxies in MKW/AWM Clusters Spiral Galaxies in MKW/AWM Clusters

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aps..mar..j504w&link_type=abstract

American Physical Society, Annual March Meeting, March 17-21, 1997, abstract #J5.04

Physics

Scientific paper

Observations have been made of the neutral hydrogen content of more than 170 galaxies within MKW 4, MKW 7, MKW 8, MKW 9, MKW 11, AWM 1, AWM 3, AWM 4, and AWM 5. This sample of nine clusters is representative of the general class of poor clusters identified by MKW and AWM in that they all contain D-- or cD--like dominant galaxies at their dynamical centers. We examine the neutral hydrogen (HI) content of the spiral members in these systems as a function of the local and global properties of the cluster, i.e., galaxy density, x-ray intra cluster gas pressure, x-ray and optical luminosities, and compare our findings with the HI properties of similar galaxies in rich clusters and loose groups of galaxies.

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