Elliptical Galaxy Halo Masses from Internal Kinematics

dc.date.accessioned2020-08-04T21:51:07Z
dc.date.accessioned2022-10-18T23:15:52Z
dc.date.available2020-08-04T21:51:07Z
dc.date.available2022-10-18T23:15:52Z
dc.date.created2020-08-04T21:51:07Z
dc.date.issued2006
dc.identifierhttp://hdl.handle.net/10533/242632
dc.identifier15010003
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4473922
dc.description.abstractThe halo masses of nearby individual elliptical galaxies can be estimated by using the kinematics of their stars, planetary nebulae, and globular clusters -- ideally in combination. With currently improving coverage of galaxies of ordinary luminosities an
dc.languageeng
dc.publisherMamon, G.
dc.publisherCombes, F.
dc.publisherParis
dc.relationhttps://arxiv.org/abs/astro-ph/0510183
dc.relationinstname: ANID
dc.relationreponame: Repositorio Digital RI2.0
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleElliptical Galaxy Halo Masses from Internal Kinematics
dc.typeCapitulo de libro


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