Maximal Halos in High-Luminosity Spiral Galaxies

Simple item page
dc.creatorSalucci, P.
dc.creatorPersic, M.
dc.date1999-03-29
dc.date.accessioned2026-07-07T02:31:01Z
dc.date.available2026-07-07T02:31:01Z
dc.descriptionWe test the halo dominated mass model, recently proposed for high-luminosity galaxies by Courteau & Rix (1998), against rotation velocity data for a large sample of L_* spirals. We find that this model does not reproduce the general kinematic properties required. The alternative disc dominated model, on the contrary, easily fits the data.
dc.description5 pages, 3 figures; A&A, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9903432
dc.identifierhttp://arxiv.org/abs/astro-ph/9903432
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14021
dc.subjectAstrophysics
dc.titleMaximal Halos in High-Luminosity Spiral Galaxies
dc.typetext

Files

Collections

arXiv