Chemical Analysis of the Brightest Star of the Cetus II Ultrafaint Dwarf Galaxy Candidate
We present a detailed chemical abundance analysis of the brightest star in the ultrafaint dwarf (UFD) galaxy candidate Cetus II from high-resolution Magellan/MIKE spectra. For this star, DES J011740.53-173053, abundances or upper limits of 18 elements from carbon to europium are derived. Its chemica...
Príomhchruthaitheoirí: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Formáid: | Alt |
Teanga: | English |
Foilsithe / Cruthaithe: |
IOP Publishing
2023-01-01
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Sraith: | The Astrophysical Journal |
Ábhair: | |
Rochtain ar líne: | https://doi.org/10.3847/1538-4357/ad0385 |