The stability of Bondi accretion

Details The stability of Bondi accretion The stability of Bondi accretion

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....73..171g&link_type=abstract

Astronomy and Astrophysics, vol. 73, no. 1-2, Mar. 1979, p. 171-173.

Astronomy and Astrophysics

Astrophysics

33

Critical Flow, Deposition, Flow Stability, Linearity, Subsonic Flow, Adiabatic Conditions, Boundaries, Boundary Conditions, Equations Of Motion, Flux Density, Gravitation

Scientific paper

The linear stability problem for Bondi (1952) accretion is solved for the case of arbitrary rather than spherically symmetric perturbations. Critical Bondi accretion is shown to be stable with respect to all perturbations. It is also found that subsonic Bondi accretion is stable for boundary conditions that are reasonable in a defined sense, particularly for those conditions that might be used in numerical calculations of accretion flows.

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