Caustic rings of dark matter

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Details

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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