Astronomy and Astrophysics – Astrophysics
Scientific paper
1995-05-05
Astron.Astrophys.303:721,1995
Astronomy and Astrophysics
Astrophysics
9 pages, uuencoded PostScript file including figures, to appear in Astronomy and Astrophysics
Scientific paper
We explore a series expansion method to calculate the modes of oscillations for a variety of uniformly rotating finite disks, either with or without a dark halo. Since all models have the same potential, this survey focuses on the role of the distribution function in stability analyses. We show that the stability behaviour is greatly influenced by the structure of the unperturbed distribution, particularly by its energy dependence. In addition we find that uniformly rotating disks with a halo in general can feature spiral-like instabilities.
Dejonghe Herwig
Vauterin P.
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