Elemental abundances of low-mass stars in the young clusters 25 Orionis andλ Orionis

2011/03/16 by K. Biazzo, S. Randich, F. Palla +2 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Homogeneous #O-type star #Spectral line #Star cluster #Stars #Stellar atmosphere #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201116621

Accepted by Astronomy and Astrophysics. 14 pages, 10 figures, 7 tables

arxiv created 2011/03/16 · openalex publication_date 2011/04/04 · arxiv updated 2015/05/27 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We aim to derive the chemical pattern of the young clusters 25 Orionis and λ Orionis through homogeneous and accurate measurements of elemental abundances.

Citations

• Sequentially triggered star formation in OB associations
• The Substellar Population of the Young Cluster λ Orionis
• On the Structure of the Orion A Cloud and the Formation of the Orion Nebula Cluster
• The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis
• ABUNDANCE RATIOS AND GALACTIC CHEMICAL EVOLUTION
• The chemical composition of the Orion star forming region

Cited by

• Elemental abundances of low-mass stars in nearby young associations:AB Doradus, Carina Near and Ursa Major

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