Exploring Group Halos Using Galaxy Dynamics

Details Exploring Group Halos Using Galaxy Dynamics Exploring Group Halos Using Galaxy Dynamics

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sgdh.conf..230w&link_type=abstract

THE SHAPES OF GALAXIES AND THEIR DARK HALOS. Proceedings of the Yale Cosmology Workshop. Held 28-30 May 2001 in New Haven, Conne

Physics

Scientific paper

I investigate some characteristics of dark matter in the Local Group and the nearby Sculptor Group. I find that there is no evidence for an extended dark matter halo around the Local Group. In addition, the angular momentum of the visible matter in the Sculptor Group is consistent with having been produced by tidal interaction among the galaxies, which indicates that the dark matter and luminous matter angular momenta are aligned.

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