Self-similar flow for spherically symmetric accretion with allowance for a pressure gradient

Details Self-similar flow for spherically symmetric accretion with allowance for a pressure gradient Self-similar flow for spherically symmetric accretion with allowance for a pressure gradient

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977afz....13..535k&link_type=abstract

Astrofizika, vol. 13, Aug. 1977, p. 535-541. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Gravitational Fields, Interstellar Gas, Stellar Mass Accretion, Asymptotic Series, Deposition, Dynamic Models, Gas Dynamics, Isentrope, Mach Number, Pressure Gradients, Shock Waves

Scientific paper

A self-similar unsteady-state solution is obtained for the problem of spherical accretion in the gravitational field of a point mass. Constant finite mass flows are specified at infinity and at the center, with the flow at infinity greater than at the center. The pressure gradient throughout space, including the region ahead of some shock front, is taken into account. The problem is also solved for an adiabatic exponent of 5/3.

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