Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..927s&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Dec. 15, 1984, p. 927-932.
Astronomy and Astrophysics
Astronomy
13
Angular Momentum, Stellar Gravitation, Stellar Mass Accretion, Stellar Rotation, B Stars, Density (Mass/Volume), Giant Stars, Gradients, Neutron Stars, O Stars, Stellar Evolution, Stellar Winds
Scientific paper
The problem of accretion from an inhomogeneous medium is examined. A scenario in which angular momentum can be deposited into the gravitating body, from a medium containing a density gradient, is proposed. The obtained equations are solved under certain simplifying assumptions. In a different regime of flow, it is suggested that angular momentum can be accreted via a displaced accretion line, within the accretion cone, in the classical Bondi-Hoyle picture.
Livio Mario
Soker Noam
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