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Halo-stripping in Galactic Collisions | Peter J. S. Watson
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18 Jul 1996 | Subject: | astro-ph | Affiliation: | Carleton University | Abstract: | 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. | Source: | arXiv, astro-ph/9607090 | Services: | Forum | Review | PDF | Favorites |
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