Halo-stripping in Galactic Collisions

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dc.creatorWatson, Peter J. S.
dc.date1996-07-18
dc.date.accessioned2026-07-07T02:21:37Z
dc.date.available2026-07-07T02:21:37Z
dc.descriptionGalactic 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.
dc.description10 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/9607090
dc.identifierhttp://arxiv.org/abs/astro-ph/9607090
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10569
dc.subjectAstrophysics
dc.titleHalo-stripping in Galactic Collisions
dc.typetext

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