Planet formation in binary stars: The case of Cephei

Astronomy and Astrophysics

Volumn 486, Issue 2, 2008, Pages 617-628

  Kley, W ^a   Nelson, R P ^b  

^a UNIVERSITY OF TÜBINGEN   (Germany)

^b QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

Author keywords

Hydrodynamics; Methods: numerical; Planets and satellites: formation; Stars: binaries: general

Indexed keywords

ARSENIC COMPOUNDS; ASTRONOMY; FLUID MECHANICS; PERTURBATION TECHNIQUES; ROCKETS; SEPARATION; SPACECRAFT OBSERVATORIES; STARS; TWO DIMENSIONAL;

ASTRONOMICAL UNIT (AU); BINARY PARAMETERS; BINARY STARS; BINARY SYSTEMS; CIRCULAR ORBITS; CO PLANARITY; ECCENTRICITY (ECC); EMBEDDED CORES; EQUILIBRIUM STRUCTURES; EVOLUTION (CO); GRAVITATIONAL PERTURBATIONS; HYDRODYNAMIC SIMULATIONS; ORBITAL ECCENTRICITY; ORBITAL EVOLUTIONS; PLANET FORMATION; SEMI-MAJOR AXIS (SMA); SPIRAL ARMS; TWO-DIMENSIONAL (2D);

FLUID DYNAMICS;

EID: 47249096579     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079324     Document Type: Article

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