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 |
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Pages (from-to) | 69 - 72 |
Number of pages | 4 |
Journal | The Astrophysical Journal |
Volume | 655 |
Issue number | 2 |
DOIs | |
Publication status | Published - 2007 |