The statistically specific angular momentum of gas in a stellar cluster

Details The statistically specific angular momentum of gas in a stellar cluster The statistically specific angular momentum of gas in a stellar cluster

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64.1176i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Nov.-Dec. 1987, p. 1176-1183. In Russian.

Astronomy and Astrophysics

Astronomy

Angular Momentum, Gas Dynamics, Interstellar Matter, Star Clusters, Statistical Analysis, Stellar Mass Ejection, Black Holes (Astronomy), Maxwell-Boltzmann Density Function

Scientific paper

The value of the specific angular momentum of gas, which is formed and stored within a quasi-spherical, nonrotating cluster of stars losing their material, is evaluated. It is shown that in stationary clusters, the probability that the gas component of a particular cluster has some value of specific angular momentum is described by the Maxwellian distribution function. Mean regular shift and statistical dispersion of this distribution are calculated. The probability of finding a gas disc structure rotating around a black hole, which is possibly situated in the centre of the cluster, is evaluated.

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