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arXiv · astro-ph/0501070

High Mach-number Bondi--Hoyle--Lyttleton flow around a small accretor

Richard Edgar
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Abstract

In this paper, we discuss a two-dimensional numerical study of isothermal high Mach number Bondi--Hoyle--Lyttleton flow around a small accretor. The flow is found to be unstable at high Mach numbers, with the instability appearing even for a larger accretor. The instability appears to be the unstable radial mode of the accretion column predicted by earlier analytic work.

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Richard Edgar. 2005-01-05. High Mach-number Bondi--Hoyle--Lyttleton flow around a small accretor. https://doi.org/10.1051/0004-6361%3A20042067

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