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Acceleration, radiation and precession in SS 433Some theoretical problems posed by the observations of SS 433 are considered. The monoenergetic beams point toward a gas-dynamic acceleration process. In this model the collimation implies that the acceleration occurs in a region of slab symmetry, possibly the surface layers of an accretion disk. The 164 day rotation of the beam pattern may be explained as a precession period.
Document ID
19800047775
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Katz, J. I.
Date Acquired
August 10, 2013
Publication Date
March 15, 1980
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
80A31945
Funding Number(s)
CONTRACT_GRANT: NSF AST-78-15431
CONTRACT_GRANT: NSG-7341
Distribution Limits
Public
Copyright
Other

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