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The Riemann disks. II - StabilityThe Riemann disks are the two-dimensional analogs of the Riemann S-type ellipsoids. They form a simple yet rich family of galactic bar models. A method is developed to find their normal modes to arbitrary order, and the stability analysis is carried out for all modes with order not greater than 5.
Document ID
19830061834
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/161226
Authors
Weinberg, M. D. (MIT Cambridge, MA, United States)
Date Acquired
August 11, 2013
Publication Date
August 15, 1983
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 271
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
83A43052
Funding Number(s)
CONTRACT_GRANT: NGL-22-609-638
CONTRACT_GRANT: NSF AST-81-20765
CONTRACT_GRANT: NSG-7643
Distribution Limits
Public
Copyright
Other

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