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DISTRIBUTION OF ACCRETING GAS AND ANGULAR MOMENTUM ONTO CIRCUMPLANETARY DISKS

Author
TANIGAWA, Takayuki1 2 ; OHTSUKI, Keiji1 3 4 ; MACHIDA, Masahiro N5
[1] Center for Planetary Science, Kobe University, Kobe, Japan
[2] Institute of Low Temperature Science, Hokkaido University, Sapporo, Japan
[3] Department of Earth and Planetary Sciences, Kobe University, Kobe, Japan
[4] Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, United States
[5] Department of Earth and Planetary Sciences, Graduate School of Sciences. Kyushu University, Fukuoka, Japan
Source

The Astrophysical journal. 2012, Vol 747, Num 1 ; 47.1-47.16 ; 1 ; ref : 1/4 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
hydrodynamics methods: numerical planets and satellites: formation protoplanetary disks shock waves
Keyword (fr)
Accrétion Cosmogonie planétaire Disque accrétion Ecoulement gaz Fonction masse Loi puissance Modèle hydrodynamique Moment cinétique Méthode numérique Nébuleuse proto planétaire Onde choc Planète géante Point Lagrange Simulation numérique Sphère
Keyword (en)
Accretion Planetary cosmogony Accretion disks Gas flow Mass function Power law Hydrodynamic model Angular momentum Numerical method Proto planetary nebula Shock waves Giant planet Lagrange point Digital simulation Spheres
Keyword (es)
Cosmogonía planetaria Función masa Ley poder Método numérico Nebulosa proto planetaria Planeta gigante Punto Lagrange
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
25564521

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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