A model of accretion of small bodies onto a binary system

Details A model of accretion of small bodies onto a binary system A model of accretion of small bodies onto a binary system

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983poast..31...19a&link_type=abstract

Postepy Astronomii (ISSN 0032-5414), vol. 31, Jan.-Mar. 1983, p. 19-34. In Polish.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Binary Stars, Molecular Clouds, Stellar Evolution, Stellar Mass Accretion, Angular Momentum, Mass Ratios, Stellar Structure

Scientific paper

A numerical model of the accretion process of matter falling from an outer, flattened accretion cloud onto a binary system with given masses and geometrical parameters is presented. The accretion process is sensitive to the mass ratio of two components of the system and the orbital angular momentum of the infalling matter. The main result of the present paper is the observation of the mass equalizing effect of accretion: the less massive component can accrete more matter than the more massive one.

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