2013/07/26 by B. Goldman, S. Röser, E. Schilbach +26 · 1 citation
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Cluster (spacecraft) #Computer science #Galaxy #Gamma-ray bursts and supernovae #Initial mass function #Luminosity #Physics #Proper motion #Sky #Star cluster #Star formation #Stars #Stellar mass #Stellar, planetary, and galactic studies #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201321727
19 pages, 16 figures, 6 tables, including a table describing all Hyades candidates available only as file table6.csv and at CDS, and a table describing the new candidates in the text and as table5.tex; accepted by A&A
openalex publication_date 2013/07/26 · arxiv created 2013/07/30 · arxiv updated 2015/06/16 · openalex created_date 2022/10/04 · openalex updated_date 2026/08/05
Aims. The Hyades cluster is an ideal target to study the dynamical evolution of a star cluster over the entire mass range due to its intermediate age and proximity to the Sun.