Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
The smallest satellites of the Milky Way ceased forming stars during the epoch of reionization and thus provide archaeological access to galaxy formation at z > 6. Numerical studies of these ultrafaint dwarf galaxies (UFDs) require expensive cosmological simulations with high mass resolution that...
| Main Authors: | , , , , , , |
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| Other Authors: | |
| Format: | Article |
| Published: |
Oxford University Press (OUP)
2019
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| Online Access: | https://hdl.handle.net/1721.1/121212 |