2013/08/01 by A. Sicilia‐Aguilar, Aurora Sicilia-Aguilar, Jinyoung Serena Kim +6 · 1 citation
Physics and Astronomy · #Accretion (finance) #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Brown dwarf #Physics #Population #Protoplanetary disk #Radiative transfer #Stars #Stellar, planetary, and galactic studies #T Tauri star #astro-ph.EP #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201321867
21 pages, 16 figures, plus appendix with tables and figures. Accepted by A&A
arxiv created 2013/08/01 · openalex publication_date 2013/08/05 · arxiv updated 2015/06/16 · openalex created_date 2022/09/28 · openalex updated_date 2026/08/04
Aims. We present a study of accretion and protoplanetary disks around M-type stars in the 4 Myr-old cluster Tr 37. With a well-studied solar-type population, Tr 37 is a benchmark for disk evolution.