On the effects of compression of a gaseous disc by thermal and dynamical pressures of intergalactic gas

Details On the effects of compression of a gaseous disc by thermal and dynamical pressures of intergalactic gas On the effects of compression of a gaseous disc by thermal and dynamical pressures of intergalactic gas

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..211k&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

1

Cosmic Gases, Disk Galaxies, Galactic Clusters, Galactic Evolution, Intergalactic Media, Interstellar Gas, Compressibility Effects, Dynamic Pressure, Gas Pressure, Molecular Clouds

Scientific paper

The authors consider a galaxy moving in a cluster of galaxies and study the effects of compression of the gas disc by both thermal and dynamical pressures of intergalactic gas. As the result of compression, massive gas clouds are formed. They are not stripped by dynamical pressure of the intergalactic gas but stay in the galaxy until they are disrupted by formation of massive stars.

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