2014/05/26 by L. Spina, S. Randich, F. Palla +38 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph.SR #msc:85A04
paper · pdf · doi:10.1051/0004-6361/201423527
published as A&A 567, A55 (2014) · 13 pages, 10 figures, 7 tables, Accepted for publication in Astronomy & Astrophysics
arxiv created 2014/05/26 · openalex publication_date 2014/05/26 · arxiv updated 2014/09/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. Knowledge of the abundance distribution of star forming regions and young clusters is critical to investigate a variety of issues, from triggered star formation and chemical enrichment by nearby supernova explosions to the ability to form planetary systems. In spite of this, detailed abundance studies are currently available for relatively few regions.