The surface brightness of H I-deficient galaxies in the Virgo Cluster

Details The surface brightness of H I-deficient galaxies in the Virgo Cluster The surface brightness of H I-deficient galaxies in the Virgo Cluster

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...194...77p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 194, no. 1-2, April 1988, p. 77, 78.

Astronomy and Astrophysics

Astrophysics

4

Brightness Distribution, H I Regions, Spiral Galaxies, Virgo Galactic Cluster, Galactic Evolution, Star Formation

Scientific paper

The three general schemes for the origin of H I-deficient galaxies, viz. primordial deficiency, direct gas loss and increased astration, are expected to lead to qualitatively different predictions for the galaxies' surface brightnesses. A sample of H I-deficient galaxies in the Virgo Cluster are shown to have lower deficient brightnesses than non-deficient galaxies. This suggests that the galaxies have been deficient in H I for a significant fraction of their lifetimes, possibly since the time of disc formation.

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