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Red Galaxies Growing in Dark Matter Halos
| Content Provider | Scilit |
|---|---|
| Author | Brown, Michael J. I. |
| Copyright Year | 2009 |
| Description | 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. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/7687B3A6F7464F2AE3DACEEBE0457BB2/S1743921310008409a.pdf/div-class-title-red-galaxies-growing-in-dark-matter-halos-div.pdf |
| Ending Page | 87 |
| Page Count | 1 |
| Starting Page | 87 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s1743921310008409 |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | H15 |
| Volume Number | 5 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2009-11-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Astronomy and Astrophysics Elliptical and Lenticular Evolution ) Dark Matter |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
