The structure of the accretion disc boundary layer around a rotating, non-magnetized star

Details The structure of the accretion disc boundary layer around a rotating, non-magnetized star The structure of the accretion disc boundary layer around a rotating, non-magnetized star

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.204....9r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 204, no. 1, p. 9-18.

Statistics

Computation

1

Accretion Disks, Boundary Layers, Stellar Rotation, Angular Velocity, Boundary Conditions, Computational Astrophysics

Scientific paper

Consideration is given to the process of disk accretion onto rotating nonmagnetized stars. A closed system of equations is written for the boundary layer that exists between the Keplerian outer part of the disk and the more slowly rotating star surface. Under certain simplifying assumptions, the system is solved numerically for the principal physical variables. An energy conservation equation is employed to determine the boundary layer radiation intensity.

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