Stationary spherical accretion into black holes. I - Equations of structure

Details Stationary spherical accretion into black holes. I - Equations of structure Stationary spherical accretion into black holes. I - Equations of structure

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.194..475t&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 194, Feb. 1981, p. 475-484.

Astronomy and Astrophysics

Astronomy

45

Black Holes (Astronomy), Stellar Mass Accretion, Stellar Structure, Optical Thickness, Relativistic Effects, State Vectors

Scientific paper

A general set of equations governing time-independent spherical accretion into black holes is formulated. The equations are fully general relativistic and are applicable to optically thick regions, optically thin regions, and the transition regions which join them. The radiation is treated using frequency-integrated moments. The full, infinite series of moment equations is given; the user of the formalism can truncate the series wherever he wishes.

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