2014/04/28 by Cyril Georgy, C. Georgy, A. Granada +11 · 2 citations
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Cluster (spacecraft) #Geometry #Magnitude (astronomy) #Metallicity #Open cluster #Physics #Rotation (mathematics) #Stars #Stellar evolution #Stellar rotation #Stellar, planetary, and galactic studies #Surface gravity #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201423881
16 pages, 16 figures, accepted for publication in A&A
arxiv created 2014/04/28 · openalex publication_date 2014/04/29 · arxiv updated 2014/06/04 · openalex created_date 2022/09/16 · openalex updated_date 2026/08/01
Context. Constraints on stellar models can be obtained from observations of stellar populations, provided the population results from a well defined star formation history.