The formation of very wide binaries during the star cluster dissolution phase

Monthly Notices of the Royal Astronomical Society

Volumn 404, Issue 4, 2010, Pages 1835-1848

  Kouwenhoven, M B N ^a,b   Goodwin, S P ^a   Parker, Richard J ^a   Davies, M B ^c   Malmberg, D ^a   Kroupa, P ^d  

^a PEKING UNIVERSITY   (China)

^b UNIVERSITY OF SHEFFIELD   (United Kingdom)

^c LUND UNIVERSITY   (Sweden)

^d UNIVERSITY OF BONN   (Germany)

Author keywords

Binaries: general; Galaxies: star clusters; Methods: N body simulations

Indexed keywords

PHASE SPACE METHODS; STARS;

BINARIES:GENERAL; BINARY FRACTION; DYNAMICAL INTERACTIONS; GALACTIC FIELDS; GALACTIC HALO; GALAXIES: STAR CLUSTERS; METHODS:N-BODY SIMULATIONS; SEMIMAJOR AXIS; STAR CLUSTERS; STARS FORMATION;

DISSOLUTION;

EID: 77953563445     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16399.x     Document Type: Article

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