Cosmic evolution of stellar quenching by AGN feedback: clues from the Horizon-AGN simulation
The observed massive end of the local galaxy stellar mass function is steeper than its predicted dark matter (DM) halo counterpart in the standard $\Lambda $CDM paradigm. We investigate how active galactic nuclei (AGN) feedback can account for such a reduction in the stellar content of massive galax...
| Main Authors: | , , , , , , , , , , |
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| Format: | Journal article |
| Published: |
Oxford University Press
2017
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