Dark Matter Halos around Galaxies

Simple item page
dc.creatorSalucci, Paolo
dc.creatorPersic, Massimo
dc.date1997-03-05
dc.date.accessioned2026-07-07T02:23:02Z
dc.date.available2026-07-07T02:23:02Z
dc.descriptionWe 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.
dc.description27 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
dc.identifierhttps://arxiv.org/abs/astro-ph/9703027
dc.identifierhttp://arxiv.org/abs/astro-ph/9703027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11095
dc.subjectAstrophysics
dc.titleDark Matter Halos around Galaxies
dc.typetext

Files

Collections

arXiv