Halo-stripping in Galactic Collisions

Details Halo-stripping in Galactic Collisions Halo-stripping in Galactic Collisions

1996-07-18

arxiv.org/abs/astro-ph/9607090v1

Astronomy and Astrophysics

Astrophysics

10 pages, 1 figure

Scientific paper

Galactic collisions are normally modeled in a CDM model by assuming the DM
consists of a small number of very massive objects. This note shows that the
behaviour of a CDM halo during collisions depends critically on the mass of the
particles that make it up, and in particular, all halo particles below a
certain characteristic mass are likely to be lost.

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