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Open Accesshttps://doi.org/10.3847/2515-5172/abfdbe
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Cite Journal: Research Notes of the AAS |  Publication Date: May 1, 2021 |
 License type: CC BY 4.0 |
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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