Pseudo-Schwarzschild Description of Accretion-Powered Spherical Outflow

Details Pseudo-Schwarzschild Description of Accretion-Powered Spherical Outflow Pseudo-Schwarzschild Description of Accretion-Powered Spherical Outflow

2002-12-10

arxiv.org/abs/astro-ph/0212217v1

International Journal of Modern Physics D, 2002,Volume 11, Issue 08, pp. 1285-1303

Astronomy and Astrophysics

Astrophysics

24 pages. 6 black and white post-script figures. Published in International Journal of Modern Physics D (IJMPD)

Scientific paper

10.1142/S0218271802002268

Using two different pseudo-Schwarzschild potentials proposed by Artemova et. al,$^{1}$ we formulate and solve the equations governing spherically symmetric transonic inflow and outflow in presence of a relativistic hadronic pressure mediated steady, standing, spherical shock around the central compact object and then we self-consistently connect the accretion-wind solutions to calculate the mass outflow rate $R_{\dot m}$ in terms of minimum number of flow parameters. Also we study the dependence of this rate on various boundary conditions governing the flow.

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