CHEMICAL SIGNATURES OF THE FIRST GALAXIES: CRITERIA FOR ONE-SHOT ENRICHMENT
We utilize metal-poor stars in the local, ultra-faint dwarf galaxies (UFDs; L [subscript tot] ≤ 10[superscript 5] L [subscript ☉]) to empirically constrain the formation process of the first galaxies. Since UFDs have much simpler star formation histories than the halo of the Milky Way, their stellar...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
IOP Publishing
2014
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| Online Access: | http://hdl.handle.net/1721.1/88430 https://orcid.org/0000-0002-2139-7145 |