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Pressure gradient torque in highly supersonic nonaxisymmetric accretionThe contribution of a pressure gradient torque to the angular momentum transfer rate in highly supersonic nonaxisymmetric accretion flows is considered. This study takes into account the contribution due to the pressure variation in the postaccretion-shock region which is significant for high Mach number accretion. For the case of accretion flow with Mach (infinity) of not less than 5, the overall accretion torque is shown to approach a constant value.
Document ID
19890056874
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ho, Cheng
(Los Alamos National Laboratory NM, United States)
Taam, Ronald E.
(Northwestern University Evanston, IL, United States)
Fryxell, Bruce A.
(Chicago, University IL, United States)
Matsuda, Takuya
(Los Alamos National Lab. NM, United States)
Koide, Hiroshi
(Kyoto University Japan)
Date Acquired
August 14, 2013
Publication Date
June 15, 1989
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 238
ISSN: 0035-8711
Subject Category
Astrophysics
Accession Number
89A44245
Funding Number(s)
CONTRACT_GRANT: NSF AST-86-08291
CONTRACT_GRANT: NAGW-768
Distribution Limits
Public
Copyright
Other

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