The Surface Abundances of Maia Revisited
Research Notes of the AAS（2021）
摘要
Abundances for 20 chemical elements are derived for Maia, the fourth brightest member of the Pleiades, using updated atomic data. Maia does not seem to be a typical helium-weak star nor a classical HgMn star. Instead Maia might be related to the phosphorus and gallium-rich stars.
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