Chemical Abundance Signature of J0023+0307: A Second-generation Main-sequence Star with [Fe/H]
We present a chemical abundance analysis of the faint halo metal-poor main-sequence star J0023+0307, with [Fe/H] <-6.3, based on a high-resolution (R ∼ 35,000) Magellan/MIKE spectrum. The star was originally found to have [Fe/H] <-6.6 based on a Ca ii K measurement in an R ∼ 2500 spectrum. No...
| Main Authors: | , , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
American Astronomical Society
2020
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| Online Access: | https://hdl.handle.net/1721.1/128722 |