The evolution of binary star clusters and the nature of NGC 2136/NGC 2137

Monthly Notices of the Royal Astronomical Society

Volumn 374, Issue 3, 2007, Pages 931-940

  Portegies Zwart, S F ^a,b   Rusli, S P ^c  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b UNIVERSITY OF AMSTERDAM   (Netherlands)

^c BANDUNG INSTITUTE OF TECHNOLOGY   (Indonesia)

Author keywords

Galaxies: star clusters; Globular clusters: individual: NGC 2136; Globular clusters: individual: NGC 2137; Gravitation; Methods: N body simulations; Stellar dynamics

Indexed keywords

ANGULAR MOMENTUM; MASS TRANSFER; SEPARATION; SUPERNOVAE;

BINARY STAR; GALAXIES: STAR CLUSTERS; GLOBULAR CLUSTER: INDIVIDUAL: NGC 2136; GLOBULAR CLUSTER: INDIVIDUAL: NGC 2137; GLOBULAR CLUSTERS: INDIVIDUAL; MASS LOSS; METHODS:N-BODY SIMULATIONS; STAR CLUSTERS; STELLAR DYNAMICS;

GRAVITATION;

EID: 33846172659     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11202.x     Document Type: Article

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