M/L in individual galaxies

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dc.creatorEmsellem, Eric
dc.date2006-10-27
dc.date2006-11-02
dc.date.accessioned2026-07-07T07:27:11Z
dc.date.available2026-07-07T07:27:11Z
dc.descriptionIn this short report, I briefly review, illustrate and discuss various techniques (e.g., X ray halos, lensing, kinematics) used to derive mass (hence M/L) profiles of individual galaxies.
dc.descriptionTo be published in the Proceedings of the XLIst Rencontres de Moriond, XXVIth Astrophysics Moriond Meeting: "From dark halos to light", Eds. L.Tresse, S. Maurogordato and J. Tran Thanh Van (Editions Frontieres). 10 pages, 6 figures. Updated references
dc.identifierhttps://arxiv.org/abs/astro-ph/0610833
dc.identifierhttp://arxiv.org/abs/astro-ph/0610833
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117289
dc.subjectAstrophysics
dc.titleM/L in individual galaxies
dc.typetext

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