Two phase, inward-then-outward migration of Jupiter and Saturn in the gaseous solar nebula

Astronomy and Astrophysics

Volumn 533, Issue , 2011, Pages

  Pierens, A ^a,b   Raymond, S N ^a,b  

^a OBSERVATOIRE DE BORDEAUX   (France)

^b LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

Author keywords

Accretion, accretion disks; Hydrodynamics; Methods: numerical; Planets and satellites: formation

Indexed keywords

1-D MODELS; ACCRETION , ACCRETION DISKS; ASTEROID BELT; DYNAMICAL EVOLUTION; GIANT PLANETS; GRID-BASED; ISOTHERMAL CONDITIONS; ISOTHERMAL EQUATION OF STATE; JUPITERS; METHODS: NUMERICALS; PLANETS AND SATELLITES: FORMATION; RADIATIVE PROPERTIES; SOLAR NEBULA; TERRESTRIAL PLANETS; TWO PHASE; TYPE II;

EQUATIONS OF STATE; FLUID DYNAMICS; HYDRODYNAMICS; NUMERICAL METHODS; PLANETS; SATELLITES;

INTERPLANETARY FLIGHT;

EID: 80052837359     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117451     Document Type: Article

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