2008/02/29 by R. K. S. Yadav, L. R. Bedin, G. Piotto +8 · 6 citations
Mathematics · Physics and Astronomy · #Archaeology #Astrometry #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Census #Cluster (spacecraft) #Computer science #Context (archaeology) #Field (mathematics) #Geography #Mathematics #Open cluster #Physics #Population #Sociology #Stars #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20079245
15 pages, 11 figures, 5 table. Accepted (2008 February 25) on A&A
arxiv created 2008/02/29 · openalex publication_date 2008/03/19 · arxiv updated 2009/12/01 · openalex created_date 2017/07/14 · openalex updated_date 2026/08/01
Context. The solar-age open cluster M 67 (C0847+120, NGC 2682) is a touchstone in studies of the old Galactic disk. Despite its outstanding role, the census of cluster membership for M 67 at fainter magnitudes and their properties are not well-established.