The gas content and star formation intensity in cluster galaxies

Details The gas content and star formation intensity in cluster galaxies The gas content and star formation intensity in cluster galaxies

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..757z&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Sept. 1987, p. 757-763. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

2

Disk Galaxies, Hydrogen, Interstellar Gas, Star Formation, Compressed Gas, Far Infrared Radiation, Galactic Clusters, Intergalactic Media, Pressure Effects

Scientific paper

The anomalously low H I abundance observed in many disk galaxies located in clusters may be associated with more rapid and efficient star formation. This is accelerated by the compression of a gas layer under the pressure of intergalactic gas in the cluster. The dependence of the fluxes in the H I line and in the FIR spectral region on the galaxies of the Virgo and Coma clusters is analyzed.

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