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The Surface Abundances of Maia Revisited

Richard Monier,Viktor Khalack

Research Notes of the AAS（2021）

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Abstract
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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surface abundances,maia
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