H I clouds from the standpoint of the adiabatic theory of galaxy formation

Details H I clouds from the standpoint of the adiabatic theory of galaxy formation H I clouds from the standpoint of the adiabatic theory of galaxy formation

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56..475d&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, May-June 1979, p. 475-484. In Russian.

Astronomy and Astrophysics

Astronomy

Galactic Evolution, Hydrogen Clouds, Nebulae, Adiabatic Conditions, Density Distribution, Entropy, Mass, Radio Astronomy

Scientific paper

Properties of (apparently high-velocity) H I clouds are considered from the standpoint of the evolutionary theory of galaxy formation. The density, entropy, mass, and radius of such clouds, as well as the distance to the clouds, are calculated on the assumption that the clouds are quasi-steady-state in nature. The results are compared with theoretical estimates, and the hypothesis that the H I clouds are extragalactic is shown to be in good agreement with the concepts of the evolutionary theory of galaxy formation.

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