Spiral galaxies in clusters. III - Gas-rich galaxies in the Pegasus I cluster of galaxies. IV - The H I color properties of spirals in nine clusters

Details Spiral galaxies in clusters. III - Gas-rich galaxies in the Pegasus I cluster of galaxies. IV - The H I color properties of spirals in nine clusters Spiral galaxies in clusters. III - Gas-rich galaxies in the Pegasus I cluster of galaxies. IV - The H I color properties of spirals in nine clusters

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87..725b&link_type=abstract

Astronomical Journal, vol. 87, May 1982, p. 725-738.

Astronomy and Astrophysics

Astronomy

23

Disk Galaxies, Galactic Clusters, Galactic Evolution, Hertzsprung-Russell Diagram, Hydrogen Clouds, Spiral Galaxies, Galactic Structure, Mass To Light Ratios, Neutral Gases, Star Distribution

Scientific paper

Results of a 21-cm and optical survey of disk galaxies in the vicinity of the Pegasus I cluster of galaxies is reported, in addition to the results of a 21-cm H I and UBV photometric survey of 235 disk galaxies in nine nearby clusters. A substantial number of blue, gas-rich galaxies are revealed for the Pegasus I cluster, and with few exceptions, the disk systems in the cluster retain large amounts of neutral hydrogen, which suggests that environmental processes have not yet removed substantial amounts of gas from these disk galaxies. The analysis of 235 disk galaxies in nearby clusters indicates that most of the clusters do not preferentially contain gas deficient spirals. The large amount of H I retained by the galaxies is not well correlated with color.

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