Isolated and companion young brown dwarfs in the Taurus and Chamaeleon molecular clouds
- Autor
- TAMURA, M1 ; ITOH, Y2 ; OASA, Y2 ; NAKAJIMA, T1
[1] National Astronomical Observatory, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan
[2] University of Tokyo, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan - Fuente
Science (Washington, D.C.). 1998, Vol 282, Num 5391, pp 1095-1097
- CODEN
- SCIEAS
- ISSN
- 0036-8075
- Campo Científico
- Multidisciplinary
- Editor
- American Association for the Advancement of Science, Washington, DC
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Analyse image Diagramme 2 couleurs Diagramme magnitude couleur Naine brune Nuage moléculaire Objet stellaire jeune
- Palabra clave (in)
- Image analysis Two color diagram Color-magnitude diagrams Brown dwarf stars Molecular clouds Young stellar objects
- Palabra clave (es)
- Diagrama 2 colores Objeto estelar joven
- 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 / 001E03C Stars / 001E03C21 Pre-main sequence objects, young stellar objects (yso's) and protostars (t tauri stars, orion population, herbig-haro objects, bok globules, bipolar outflows, cometary nebulae, etc.)
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D38 Interstellar medium (ism) and nebulae in milky way / 001E03D38D Molecular clouds, h2 clouds, dense clouds, and dark clouds
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 1608018
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
10.1126/science.282.5391.1095 
https://dx.doi.org/10.1126/science.282.5391.1095
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