THE RUNTS OF THE LITTER: WHY PLANETS FORMED THROUGH GRAVITATIONAL INSTABILITY CAN ONLY BE FAILED BINARY STARS
- Author
- KRATTER, Kaitlin M1 ; MURRAY-CLAY, Ruth A2 ; YOUDIN, Andrew N3
[1] Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto ON, M5S 3H4, Canada
[2] Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS-51, Cambridge, MA 02138, United States
[3] Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON, M5S 3H8, Canada - Source
The Astrophysical journal. 2010, Vol 710, Num 2, pp 1375-1386, 12 p ; 1 ; ref : 3/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- IOP, Bristol
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- binaries: general brown dwarfs planet-disk interactions planets and satellites: formation protoplanetary disks
- Keyword (fr)
- Binaire Cosmogonie planétaire Instabilité gravitationnelle Naine brune Nébuleuse proto planétaire Planète
- Keyword (en)
- Binary stars Planetary cosmogony Gravitational instability Brown dwarf stars Proto planetary nebula Planets
- Keyword (es)
- Cosmogonía planetaria Nebulosa proto planetaria
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 22995273
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
10.1088/0004-637X/710/2/1375 
https://dx.doi.org/10.1088/0004-637X/710/2/1375
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