Binaries of massive black holes in rotating clusters: Dynamics, gravitational waves, detection and the role of eccentricity

Monthly Notices of the Royal Astronomical Society

Volumn 401, Issue 4, 2010, Pages 2268-2284

  Amaro Seoane, P ^a,b   Eichhorn, C ^c,d   Porter, E K ^e   Spurzem, R ^d,f,g  

^a ALBERT EINSTEIN INSTITUT   (Germany)

^b CSIC   (Spain)

^c UNIVERSITY OF STUTTGART   (Germany)

^d ASTRONOMISCHES RECHEN INSTITUT   (Germany)

^e UNIVERSITÉ PARIS DIDEROT   (France)

^f CHINESE ACADEMY OF SCIENCES   (China)

^g PEKING UNIVERSITY   (China)

Author keywords

Black hole physics; Globular clusters: general; Gravitational waves; Stellar dynamics

Indexed keywords

ANTENNAS; BLACK HOLES; GRAVITATIONAL EFFECTS; INTERFEROMETERS; LASER INTERFEROMETRY; ROTATION; SIGNAL TO NOISE RATIO; STARS; SURVEYS;

BLACK HOLE PHYSICS; CLUSTER DYNAMICS; DYNAMICAL EVOLUTION; GLOBULAR CLUSTERS:GENERAL; GRAVITATIONAL-WAVE DETECTION; INITIAL VELOCITIES; LASER INTERFEROMETER SPACE ANTENNA; MASSIVE BLACK HOLES; ROTATING CLUSTERS; STELLAR DYNAMICS;

GRAVITY WAVES;

EID: 74549204724     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15842.x     Document Type: Article

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