The Surface Abundances of Maia Revisited
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.
- Publication:
-
Research Notes of the American Astronomical Society
- Pub Date:
- May 2021
- DOI:
- 10.3847/2515-5172/abfdbe
- Bibcode:
- 2021RNAAS...5..104M
- Keywords:
-
- Chemically peculiar stars;
- Chemical abundances;
- 226;
- 224
