A direct N-body model of core-collapse and core oscillations

Monthly Notices of the Royal Astronomical Society

Volumn 425, Issue 4, 2012, Pages 2872-2879

  Hurley, Jarrod R ^a   Shara, Michael M ^b  

^a SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^b DIVISION OF INVERTEBRATE ZOOLOGY   (United States)

Author keywords

Binaries: close; Galaxies: star clusters: general; Globular clusters: general; Methods: numerical; Stars: evolution; Stars: kinematics and dynamics

Indexed keywords

BLACK HOLES; NUMERICAL METHODS;

BINARIES: CLOSE; BODY MODELS; CORE COLLAPSE; DIRECT N; GALAXIES: STAR CLUSTERS: GENERALS; GLOBULAR CLUSTERS:GENERAL; METHOD: NUMERICAL; N-BODY SIMULATION; STAR KINEMATICS AND DYNAMICS; STAR: EVOLUTION;

STARS;

EID: 84873908505     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2012.21668.x     Document Type: Article

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