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 Boötes field and N-body simulations to argue that about 1/3 of the most luminous satellite galaxies appear to undergo merging or disruption within massive halos between z ≃ 0.9 and 0.5.
Original language | English (US) |
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Pages (from-to) | L69-L72 |
Journal | Astrophysical Journal |
Volume | 655 |
Issue number | 2 II |
DOIs | |
State | Published - Feb 1 2007 |
Externally published | Yes |
Keywords
- Galaxies: evolution
- Galaxies: halos
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science