Chemical composition of A and F dwarf members of the Coma Berenices open cluster

2007/12/03 by M. Gebran, Richard Monier, R. Monier +1 · 2 citations
Earth and Planetary Sciences · Physics and Astronomy · #Astro and Planetary Science #Astronomical and nuclear sciences #Astrophysics #Cluster (spacecraft) #Coma (optics) #Composition (language) #Computer science #Geology and Paleoclimatology Research #Linguistics #Open cluster #Operating system #Philosophy #Physics #Stars #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078807

25 pages, 20 figures

arxiv created 2007/12/03 · openalex publication_date 2007/12/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.Abundances of 18 chemical elements have been derived for 11 A (normal and Am) and 11 F dwarfs members of the Coma Berenices open cluster in order to set constraints on evolutionary models including transport processes (radiative and turbulent diffusion) calculated with the Montréal code.

Citations

• An optimal extraction algorithm for CCD spectroscopy

Cited by

• A spectroscopic study of the open cluster NGC 6475 (M 7). Chemical abundances from stars in the range Teff = 4500-10 000 K
• A Metallicity Study of F, G, K, and M Dwarfs in the Coma Berenices Open Cluster from the APOGEE Survey