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1994ApJ...426..170C - Astrophys. J., 426, 170-191 (1994/May-1)
Chemical evolution of the Orion association. II. The carbon, nitrogen, oxygen, silicon and iron abundances of main-sequence B stars.
CUNHA K. and LAMBERT D.L.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Abundances - Galaxy: Open Clusters and Associations: Individual Name: Orion I - Stars: Early-Type
Simbad objects: 20
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