High Mach-number Bondi--Hoyle--Lyttleton flow around a small accretor
arXiv:astro-ph/0501070 · doi:10.1051/0004-6361:20042067
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.
Five pages, nine figures Accepted by A&A
References in corpus (1)
Cited by in corpus (5)
- Asymmetric Accretion Flows within a Common Envelope
- The Evolution of Binaries in a Gaseous Medium: Three-Dimensional Simulations of Binary Bondi-Hoyle-Lyttleton Accretion
- Three-dimensional hydrodynamical models of wind and outburst-related accretion in symbiotic systems
- Numerical simulations of axisymmetric hydrodynamical Bondi-Hoyle accretion onto a compact object
- Dynamical friction for accelerated motion in a gaseous medium