Initial results from the Palomar Adaptive Optics Survey of Young solar-type stars: A brown dwarf and three stellar companions
- Autor
- METCHEV, Stanimir A1 ; HILLENBRAND, Lynne A1
[1] Division of Physics, Mathematics, and Astronomy, California Institute of Technology, MS 105-24, Pasadena, CA 91125, United States - Fuente
The Astrophysical journal. 2004, Vol 617, Num 2, pp 1330-1346, 17 p ; 1 ; ref : 112 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 de autor
- binaries: close instrumentation: adaptive optics stars: individual (HD 49197, HD 129333, V522 Persei, RX J0329.1+0118) stars: low-mass, brown dwarfs
- Palabra clave (fr)
- Analyse image Binaire serrée Etoile faible masse Etoile jeune Etoile type solaire Naine brune Optique adaptative
- Palabra clave (in)
- Image analysis Close binary stars Low-mass stars Young stars Solar type star Brown dwarf stars Adaptive optics
- Palabra clave (es)
- Estrella tipo solar
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C20 Normal stars (by class): general or individual / 001E03C20J Main-sequence: late-type stars (g, k, and m)
- 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
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 16525425
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
10.1086/425410 
https://dx.doi.org/10.1086/425410
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