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Fragmentation of gravitationally unstable gaseous protoplanetary disks with radiative transfer

Author
MAYER, Lucio1 2 ; LUFKIN, Graeme3 ; QUINN, Thomas4 ; WADSLEY, James5
[1] Department of Physics, Institut für Astronomie, ETH Zürich, 8093, Zürich, Switzerland
[2] Institut für Theoretische Physik, University of Zurich, 8057 Zürich, Switzerland
[3] Department of Astronomy, University of Maryland, College Park, MD 20742-2421, United States
[4] Department of Astronomy, University of Washington, Seattle, WA 98195, United States
[5] Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1, Canada
Source

The Astrophysical journal. 2007, Vol 661, Num 1 ; L77-L80 ; 2 ; ref : 1/4 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
accretion, accretion disks hydrodynamics methods : n-body simulations planetary systems: formation solar system: formation
Keyword (fr)
Cosmogonie planétaire Disque accrétion Fragmentation Nébuleuse proto planétaire Simulation numérique Système n corps Système planétaire Système solaire Transfert radiatif
Keyword (en)
Planetary cosmogony Accretion disks Fragmentation Proto planetary nebula Digital simulation N body system Planetary system Solar system Radiative transfer
Keyword (es)
Cosmogonía planetaria Nebulosa proto planetaria Sistema n cuerpos Sistema planetario
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18782516

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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