Stars and brown dwarfs in theσOrionis cluster: the Mayrit catalogue

2007/10/31 by Jose A. Caballero, J. A. Caballero · 1 citation
Medicine · Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Brown dwarf #Cluster (spacecraft) #Computer science #Context (archaeology) #Geography #Low Mass #Medicine #Open cluster #Physics #Population #Stars #Stellar classification #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20077885

accepted for publication in A&A, section 14. Online catalogs and data

arxiv created 2007/10/31 · openalex publication_date 2007/12/04 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context.The young σ Orionis cluster is an indispensable basis for understanding the formation and evolution of stars, brown dwarfs, and planetary-mass objects. Our knowledge of its stellar population is, however, incomplete.

Citations

• Discovery of a dust cloud next to σ Orionis
• Accretion in Young Stellar/Substellar Objects
• ASpitzer Space TelescopeStudy of Disks in the Young σ Orionis Cluster
• Spatial distribution of stars and brown dwarfs in σ Orionis
• The Two Micron All Sky Survey (2MASS)
• S Orionis 70: Just a Foreground Field Brown Dwarf?
• The USNO-B Catalog
• A search for substellar members in the Praesepe and σ Orionis clusters
• Are isolated planetary-mass objects really isolated?

Cited by

• Contamination by field late-M, L, and T dwarfs in deep surveys