Limiting eccentricity of subparsec massive black hole binaries surrounded by self-gravitating gas discs

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 4, 2011, Pages 3033-3041

  Roedig, C ^a   Dotti, M ^b,c   Sesana, A ^a   Cuadra, J ^b,d   Colpi, M ^c  

^a ALBERT EINSTEIN INSTITUT   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c UNIVERSITY OF MILANO BICOCCA   (Italy)

^d PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

Author keywords

Accretion, accretion discs; Black hole physics; Gravitational waves; Methods: numerical

Indexed keywords

ANTENNAS; BLACK HOLES; FREQUENCY DOMAIN ANALYSIS; GRAVITATIONAL EFFECTS; HYDRODYNAMICS; INTERFEROMETERS; LASER INTERFEROMETRY; NUMERICAL METHODS; STARS;

ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; HYDRODYNAMIC CODES; LASER INTERFEROMETER SPACE ANTENNA; MASS RATIO; MASSIVE BLACK HOLES; METHOD: NUMERICAL; SMOOTHED PARTICLE HYDRODYNAMICS; SUPERMASSIVE BLACK HOLES; TOTAL MASS;

GRAVITY WAVES;

EID: 80051819996     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18927.x     Document Type: Article

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