The mysterious origin of brown dwarfs
- Autor
- PADOAN, Paolo1 ; NORDLUND, Ake2
[1] Department of Physics, University of California, San Diego, CASS/UCSD 0424, 9500 Gilman Drive, La Jolla, CA 92093-0424, Denmark
[2] Astronomical Observatory, Niels Bohr Institute for Astronomy, Physics, and Geophysics, Juliane Maries Vej 30, 2100, Copenhagen, Denmark - Fuente
The Astrophysical journal. 2004, Vol 617, Num 1, pp 559-564, 6 p ; 1 ; ref : 64 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 stellaire Formation stellaire Fragmentation Instabilité gravitationnelle Matière interstellaire Naine brune Nuage moléculaire Proto étoile Turbulence
- Palabra clave (in)
- Star clusters Star formation Fragmentation Gravitational instability Interstellar matter Brown dwarf stars Molecular clouds Protostars Turbulence
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10B Star formation
- 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
- 16387316
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
10.1086/345413 
https://dx.doi.org/10.1086/345413
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