Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientific paper
2010-01-14
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
4 pages, 3 figures. To appear in the proceedings of IAU Symposium 262: Stellar Populations - Planning for the Next Decade
Scientific paper
In cold dark matter cosmologies, the most massive dark matter halos are predicted to undergo rapid growth at z<1. While there is the expectation that massive galaxies will also rapidly grow via merging, recent observational studies conclude that the stellar masses of the most massive galaxies grow by just 30 percent at z<1. We have used the observed space density and clustering of z<1 red galaxies in Bootes to determine how these galaxies populate dark matter halos. In the most massive dark matter halos, central galaxy stellar mass is proportional to halo mass to the power of a third and much of the stellar mass resides within satellite galaxies. As a consequence, the most massive galaxies grow slowly even though they reside within rapidly growing dark matter halos.
Brown Michael J. I.
the Bootes Field Collaborations
No associations
LandOfFree
The Slow Growth of Massive Galaxies in Rapidly Growing Dark Matter Halos does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Slow Growth of Massive Galaxies in Rapidly Growing Dark Matter Halos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Slow Growth of Massive Galaxies in Rapidly Growing Dark Matter Halos will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-567780