Angular-momentum transfer in steady-state disk accretion

Details Angular-momentum transfer in steady-state disk accretion Angular-momentum transfer in steady-state disk accretion

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977azh....54.1036g&link_type=abstract

Astronomicheskii Zhurnal, vol. 54, Sept.-Oct. 1977, p. 1036-1040. In Russian.

Astronomy and Astrophysics

Astrophysics

2

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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