Subsonic Accretion through Stellar Boundary Layers

Details Subsonic Accretion through Stellar Boundary Layers Subsonic Accretion through Stellar Boundary Layers

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...184.1302k&link_type=abstract

American Astronomical Society, 184th AAS Meeting, #13.02; Bulletin of the American Astronomical Society, Vol. 26, p.878

Astronomy and Astrophysics

Astronomy

Scientific paper

Recent progress(1,2) in the application of numerical relaxation techniques has made possible the construction of steady-state boundary-layer solutions for thin alpha-disks around accreting unmagnetized stars. Physically acceptable solutions must satisfy the constraint that the radial inflow velocity not be supersonic. Preliminary results on new models of subsonic accretion will be presented. Supported in part through KBN grant 2-1244-91-01. References 1. Paczynski, B. 1991, ApJ 370, 597-603. 2. Popham, R. & Narayan, R. 1992, ApJ 394, 255-260.

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