Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.188...75c&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 188, July 1979, p. 75-82.
Astronomy and Astrophysics
Astronomy
3
Gravitational Effects, Interstellar Gas, Stellar Gravitation, Stellar Mass Accretion, Black Holes (Astronomy), Cosmic Dust, Criteria, Density Distribution, Galactic Clusters, Hydrogen Clouds, Interstellar Matter, Star Clusters
Scientific paper
The criteria and conditions when the effects of self-gravitation of the cloud in steady spherically symmetric accretion would lead to an actual enhancement in the accretion rate and density distribution are outlined. The role of self-gravitation is not significant for stellar objects accreting from the interstellar medium but it can be for those accreting from dense cold clouds, massive black holes, stellar clusters, galaxies and clusters of galaxies accreting under a wide range of conditions.
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