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Dark-Matter in Galaxies from Gravitational Lensing and Stellar Dynamics Studies

Published online by Cambridge University Press:  21 October 2010

L. V. E. Koopmans
L. V. E. Koopmans*
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700AV, Groningen, The Netherlands; email: koopmans@astro.rug.nl
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Abstract

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Strong gravitational lensing and stellar dynamics provide two complementary methods in the study of the mass distribution of dark matter in galaxies out to redshift of unity. They are particularly powerful in the determination of the total mass and the density profile of mass early-type galaxies on kpc to tens of kpc scales, and also reveal the presence of mass-substructure on sub-kpc scale. I will shortly discuss these topics in this review.

Keywords

Galaxies: elliptical and lenticularcD – Galaxies: formation – Galaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 74
Copyright
Copyright © International Astronomical Union 2010

References

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