Dark Matter Halos around Galaxies
Astrophysics
2007-05-23 v1
Abstract
We present evidence that all galaxies, of any Hubble type and luminosity, bear the kinematical signature of a mass component distributed differently from the luminous matter. We review and/or derive the DM halo properties of galaxies of different luminosities and morphologies: spirals, LSBs, ellipticals, dwarf irregulars and dwarf spheroidals.
Cite
@article{arxiv.astro-ph/9703027,
title = {Dark Matter Halos around Galaxies},
author = {Paolo Salucci and Massimo Persic},
journal= {arXiv preprint arXiv:astro-ph/9703027},
year = {2007}
}
Comments
27 pages, latex, 18 figures. Review to appear in "Dark and Visible Matter in Galaxies". Proceedings of the Sesto DM1996 Conference Eds M. Persic & P. Salucci. ASP Proceedings Conference Series 1997 also available at ftp://galileo.sissa.it/users/ftp/pub/psrot/persucci.ps