Transfer of angular momentum during steady disk accretion

Details Transfer of angular momentum during steady disk accretion Transfer of angular momentum during steady disk accretion

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sva....21..587g&link_type=abstract

(Astronomicheskii Zhurnal, vol. 54, Sept.-Oct. 1977, p. 1036-1040.) Soviet Astronomy, vol. 21, Sept.-Oct. 1977, p. 587-589. Tra

Astronomy and Astrophysics

Astrophysics

Angular Momentum, Astrophysics, Momentum Transfer, Stellar Envelopes, Stellar Mass Accretion, Differential Equations, Mass Transfer, Steady State, Stellar Models, Time Dependence

Scientific paper

Conditions of steady-state disk accretion are considered. It is shown
that accretion may be time-independent only if there are constant
inflows of matter and angular momentum across the outer boundary of the
disk. The total input of angular momentum at this boundary is
transferred through the disk to the surface of the central star.

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