Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-05-06
Phys.Lett. B432 (1998) 139-144
Astronomy and Astrophysics
Astrophysics
12 pages, 1 figure, Latex, minor changes, version to to be published by Phys. Lett. B
Scientific paper
10.1016/S0370-2693(98)00595-4
It is shown that the infall of collisionless dark matter onto isolated
galaxies produces a series of caustic rings in the halo dark matter
distribution. The properties of these caustics are investigated. The density
profile of the caustic is derived for a specific case. Bumps in the rotation
curve of NGC 3198 are interpreted as due to caustic rings of dark matter.
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