Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-23T12:01:06.261Z Has data issue: false hasContentIssue false

Red Galaxies Growing in Dark Matter Halos

Published online by Cambridge University Press:  21 October 2010

Michael J. I. Brown
Affiliation:
School of Physics, Monash University, Clayton, Victoria 3800, Australia email: Michael.Brown@sci.monash.edu.au
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

To understand the slow growth of massive galaxies at z < 1, we have modeled how these galaxies populate dark matter halos. The models are constrained with the observed luminosity function and clustering of z < 1 red galaxies. In the most massive halos, much of the stellar mass resides within multiple satellite galaxies rather than a single central galaxy. Consequently, massive galaxies grow slowly within rapidly growing dark matter halos.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Brown, M. J. I., Zheng, Z., White, M., Dey, A., Jannuzi, B. T., Benson, A. J., Brand, K., Brodwin, M., & Croton, D. J. 2008, ApJ 682, 937CrossRefGoogle Scholar
White, M., Zheng, Z., Brown, M. J. I., Dey, A., & Jannuzi, B. T. 2007, ApJ (Letters) 655, 69CrossRefGoogle Scholar