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The stability of perfect elliptic disks. 1: The maximum streaming caseSelf-consistent distribution functions are constructed for two-dimensional perfect elliptic disks (for which the potential is exactly integrable) in the limit of maximum streaming; these are tested for stability by N-body integration. To obtain a discrete representation for each model, simulated annealing is used to choose a set of orbits which sample the distribution function and reproduce the required density profile while carrying the greatest possible amount of angular momentum. A quiet start technique is developed to place particles on these orbits uniformly in action-angle space, making the initial conditions as smooth as possible. The roundest models exhibit spiral instabilities similar to those of cold axisymmetric disks; the most elongated models show bending instabilities like those seen in prolate systems. Between these extremes, there is a range of axial ratios 0.25 approximately less than b/a approximately less than 0.6 within which these models appear to be stable. All the methods developed in this investigation can easily be extended to integrable potentials in three dimensions.
Document ID
19950029115
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Levine, Stephen E.
(Washburn Observatory, Madison, WI United States)
Sparke, Linda S.
(Washburn Observatory, Madison, WI United States)
Date Acquired
August 16, 2013
Publication Date
June 20, 1994
Publication Information
Publication: The Astrophysical Journal
Volume: 428
Issue: 2 pt
ISSN: 0004-637X
Subject Category
Astronomy
Accession Number
95A60714
Funding Number(s)
CONTRACT_GRANT: NAGW-2420
Distribution Limits
Public
Copyright
Other

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