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Establishing the relationship between galaxies and dark matter

Published online by Cambridge University Press:  01 August 2006

H. J. Mo ,
X.H. Yang ,
F.C. van den Bosch ,
Y.P. Jing  and
S.M. Weinmann
H. J. Mo
Affiliation:
Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA email: hjmo@nova.astro.umass.edu
X.H. Yang
Affiliation:
Shanghai Astronomical Observatory, Shanghai, China
F.C. van den Bosch
Affiliation:
Max-Planck-Institute for Astronomy, Heidelberg, Germany
Y.P. Jing
Affiliation:
Shanghai Astronomical Observatory, Shanghai, China
S.M. Weinmann
Affiliation:
Institute of Astronomy, Zurich, Switzerland
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Abstract

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We use two methods to establish the relationship between galaxies and dark matter halos. One is based the conditional luminosity function model, which links galaxies and dark matter halos by matching the number density and clustering properties of galaxies with those of dark matter halos in the current CDM model. The second is based on galaxy systems identified from large redshift surveys of galaxies. The galaxy – dark halo relationships established by these two methods match well, and can provide important constraints on how galaxies form and evolve in the universe.

Keywords

Galaxiesdark matterdark matter halos
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 43 - 47
Copyright
Copyright © International Astronomical Union 2007

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