Modeling the Jovian subnebula I. Thermodynamic conditions and migration of proto-satellites

Astronomy and Astrophysics

Volumn 439, Issue 3, 2005, Pages 1205-1213

  Alibert, Y ^a   Mousis, O ^a,b   Benz, W ^a  

^a UNIVERSITY OF BERN   (Switzerland)

^b OBSERVATOIRE DE BESANÇON   (France)

Author keywords

Planets and satellites: formation; Solar system: formation

Indexed keywords

ASTROPHYSICS; FUNCTIONS; SATELLITES; TURBULENT FLOW; VISCOSITY;

PLANETS AND SATELLITES: FORMATION; SOLAR SYSTEM: FORMATION;

ASTRONOMY;

EID: 24944479161     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20052841     Document Type: Article

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