Realizability of stationary spherically symmetric transonic accretion

Details Realizability of stationary spherically symmetric transonic accretion Realizability of stationary spherically symmetric transonic accretion

2002-12-28

arxiv.org/abs/astro-ph/0212558v2

Phys.Rev. E66 (2002) 066303

Astronomy and Astrophysics

Astrophysics

4 pages in REVTeX with 2 figures. Typos have been corrected and some alterations have been made in the version published in Ph

Scientific paper

10.1103/PhysRevE.66.066303

The spherically symmetric stationary transonic (Bondi) flow is considered a
classic example of an accretion flow. This flow, however, is along a
separatrix, which is usually not physically realizable. We demonstrate, using a
pedagogical example, that it is the dynamics which selects the transonic flow.

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