1999/07/02 by D. Barrado y Navascues, D. Barrado, Constantine P. Deliyannis +5
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9907026
4 Pages. Contribution to "Stellar Clusters and Association: Convection, Rotation, and Dynamos", ASP Conf. Series, in press
arxiv created 1999/07/02 · openalex publication_date 1999/07/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We have obtained high resolution spectra of ∼40 members of M35, determined the Lithium-T_\rmeff morphology and the distribution of the rotational velocity for G and K stars, and compared them to those of the Pleiades and other well-known open clusters.