Some dynamic effects that may be expected to ARISE in the motion of galaxies in a gaseous medium

Details Some dynamic effects that may be expected to ARISE in the motion of galaxies in a gaseous medium Some dynamic effects that may be expected to ARISE in the motion of galaxies in a gaseous medium

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974azh....51..721z&link_type=abstract

Astronomicheskii Zhurnal, vol. 51, July-Aug. 1974, p. 721-723. In Russian.

Astronomy and Astrophysics

Astronomy

2

Celestial Mechanics, Dynamic Characteristics, Galactic Structure, Intergalactic Media, Interstellar Gas, Astronomical Photography, Hydrogen, Spiral Galaxies, Virgo Galactic Cluster

Scientific paper

It is shown that the motion of galaxies in the intergalactic medium may lead to partial disruption of the interstellar gas layer and to gas losses in the peripheral regions of the galaxies. As a result, there may arise: an HI deficiency of the type apparently occurring in the galaxies of the Virgo cluster; a color excess which, according to Holmberg (1964), is characteristic of some spiral galaxies in Virgo; and a characteristic dust layer asymmetry, as observed in some individual galaxies.

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