2021RNAAS...5..104M

Query : 2021RNAAS...5..104M

2021RNAAS...5..104M - Research Notes of the AAS, 5, 104 (2021/May-0)

The Surface Abundances of Maia Revisited.

MONIER R. and KHALACK V.

Abstract (from CDS):

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.

Abstract Copyright: © 2021. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Chemically peculiar stars - Chemical abundances

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 * 20 Tau PM* 03 45 49.6081548365 +24 22 03.877565838 3.40 3.80 3.87 3.85 3.90 B7III 451 1
2 Cl Melotte 22 OpC 03 46 38.0 +24 10 41           ~ 3679 0

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