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Astronomy and Astrophysics

Volumn 507, Issue 1, 2009, Pages 505-511

Planet formation in highly inclined binaries

(3) Marzari, F a Thebault P b Scholl, H c

a UNIVERSITY OF PADOVA (Italy)

b OBSERVATOIRE DE PARIS (France)

c UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS (France)

Author keywords

Methods: numerical; Planetary systems: formation

Indexed keywords

3-BODY PROBLEM; BINARY SEPARATION; BINARY SYSTEMS; IMPACT VELOCITIES; MAIN PARAMETERS; METHODS: NUMERICALS; PLANET FORMATION; PLANETARY SYSTEMS: FORMATION; PLANETESIMAL DISKS; PROTOPLANETARY DISKS; PROTOPLANETS; RELATIVE VELOCITY; SEMIMAJOR AXIS; TIME-SCALES;

DISKS (STRUCTURAL COMPONENTS); NUMERICAL METHODS;

ASTRONOMY;

EID: 70449679237 PISSN: 00046361 EISSN: 14320746 Source Type: Journal
DOI: 10.1051/0004-6361/200912379 Document Type: Article

Times cited : (26)

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