The dynamics of a wind-driven shell in a steady-state accretion flow - The self-similar case

Details The dynamics of a wind-driven shell in a steady-state accretion flow - The self-similar case The dynamics of a wind-driven shell in a steady-state accretion flow - The self-similar case

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18...92g&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 92; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 3, March 1992, p. 228

Astronomy and Astrophysics

Astronomy

Interstellar Gas, Stellar Envelopes, Stellar Mass Accretion, Stellar Winds, Equations Of Motion, Gas Dynamics, Steady State

Scientific paper

Self-similar (power-law) solutions for the problem of the motion of a stellar (galactic) wind-driven shell in a steady-state accretion flow are found in the thin-layer approximation, taking gravity, counterpressure, and radiative effects into account. The properties of the power-law solutions of equations describing the steady-state accretion and the dynamics of the wind-driven envelope are analyzed.

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