Identification of a Group III CEMP-no Star in the Dwarf Spheroidal Galaxy Canes Venatici I
CEMP-no stars, a subclass of carbon-enhanced metal-poor (CEMP) stars, are one of the most significant stellar populations in galactic archeology, because they dominate the low end of the metallicity distribution function, providing information on the early star formation and chemical-evolution history of the Milky Way and its satellite galaxies
Yoon, Jinmi et al.
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2020