M/L in individual galaxies
Astrophysics
2007-05-23 v2
Abstract
In 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.
Cite
@article{arxiv.astro-ph/0610833,
title = {M/L in individual galaxies},
author = {Eric Emsellem},
journal= {arXiv preprint arXiv:astro-ph/0610833},
year = {2007}
}
Comments
To 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