Abstract
The formation and evolution of massive red galaxies form a crucial test of theories of galaxy formation based on hierarchical assembly. In this Letter we use observations of the clustering of luminous red galaxies from the Bootes field and N-body simulations to argue that about (1)/(3) of the most luminous satellite galaxies appear to 1 3 undergo merging or disruption within massive halos between and z similar or equal to 0.9 and 0.5.
| Original language | English |
|---|---|
| Pages (from-to) | 69 - 72 |
| Number of pages | 4 |
| Journal | The Astrophysical Journal |
| Volume | 655 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 2007 |
Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver