S orionis 70: Just a foreground field brown dwarf?
- Autor
- 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 - Fuente
The Astrophysical journal. 2004, Vol 604, Num 2, pp 827-831, 5 p ; 1 ; ref : 45 ref
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- University of Chicago Press, Chicago, IL
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Amas jeune Amas ouvert Etoile faible masse Etoile membre Formation stellaire Gravité surface Naine brune Système planétaire
- Palabra clave (in)
- Young cluster Open clusters Low-mass stars Member star Star formation Surface gravity Brown dwarf stars Planetary system
- Palabra clave (es)
- Cúmulo joven Estrella miembro Sistema planetario
- Clasificación
- 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
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 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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DOI
10.1086/382129 
https://dx.doi.org/10.1086/382129
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