The onset of planet formation in brown dwarf disks
- Author
- APAI, Daniel1 2 ; PASCUCCI, Ilaria1 ; BOUWMAN, Jeroen3 ; NATTA, Antonella4 ; HENNING, Thomas3 ; DULLEMOND, Cornelis P3
[1] Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, United States
[2] NASA Astro biology Institute, NASA Ames Research Center, Moffett Field, CA 94035, United States
[3] Max Planck Institute for Astron omy, Königstuhl 17, Heidelberg, 69117, Germany
[4] Osservatorio Astrofisico di Arcetri, Institute Nazionale di Astrofisica, Largo E. Fermi 5, 50125 Firenze, Italy - Source
Science (Washington, D.C.). 2005, Vol 310, Num 5749, pp 834-836, 3 p
- CODEN
- SCIEAS
- ISSN
- 0036-8075
- Scientific domain
- Multidisciplinary
- Publisher
- American Association for the Advancement of Science, Washington, DC
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Cosmogonie planétaire Cristallisation Disque circumstellaire Grain poussière Masse stellaire Naine brune Nébuleuse proto planétaire Spectre IR
- Keyword (en)
- Planetary cosmogony Crystallization Circumstellar disks Dust grain Stellar mass Brown dwarf stars Proto planetary nebula Infrared spectra
- Keyword (es)
- Cosmogonía planetaria Mota polvo Nebulosa proto planetaria
- 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 / 001E03C Stars / 001E03C82 Extrasolar planetary systems / 001E03C82J Infrared excess ; debris disks ; protoplanetary disks ; exo-zodiacal dust
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17241328
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.1118042 
https://dx.doi.org/10.1126/science.1118042
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