Hydrodynamical Studies of Wind Accretion onto Compact Objects: Two‐dimensional Calculations
Year: 1997
Type: article
Abstract: We present the results of hydrodynamical simulations of nonaxisymmetric gas flow past a gravitating compact object in two dimensions. Calculations were performed with uniform flow as well as with transverse velocity and density gradients. We find that the flow is highly nonsteady, exhibiting the "flip-flop" behavior seen in previous studies, in which accretion disks form with alternating directions of rotation. We investigate the periodicity of the flip-flop behavior and study the effects of spatial resolution on the results. We find that the flip-flop motion creates accretion torques that, in some cases, may be large enough to explain the erratic spin behavior observed in Be-type X-ray pulsars.
Source: The Astrophysical Journal
DOI: 10.1086/303835
Authors: J. S. Benensohn, D. Q. Lamb, R. E. Taam
Institutions: University of Chicago, Northwestern University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2015733693
