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S orionis 70: Just a foreground field brown dwarf?

Author
BURGASSER, Adam J1 ; KIRKPATRICK, J. Davy2 ; MCGOVERN, Mark R1 ; MCLEAN, Ian S1 ; PRATO, L1 ; REID, I. Neill3
[1] Department of Physics and Astronomy, University of California at Los Angeles, Los Angeles, CA, 90095-1562, United States
[2] Infrared Processing and Analysis Center, M/S 100-22, California Institute of Technology, Pasadena, CA 91125, United States
[3] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States
Source

The Astrophysical journal. 2004, Vol 604, Num 2, pp 827-831, 5 p ; 1 ; ref : 45 ref

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Amas jeune Amas ouvert Etoile faible masse Etoile membre Formation stellaire Gravité surface Naine brune Système planétaire
Keyword (en)
Young cluster Open clusters Low-mass stars Member star Star formation Surface gravity Brown dwarf stars Planetary system
Keyword (es)
Cúmulo joven Estrella miembro Sistema planetario
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C20 Normal stars (by class): general or individual / 001E03C20V Low luminosity stars, subdwarfs, and brown dwarfs

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D20 Stellar clusters and associations / 001E03D20D Open clusters in the milky way

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16060287

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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