Evolution of binary black holes in self gravitating discs: Dissecting the torques

Astronomy and Astrophysics

Volumn 545, Issue , 2012, Pages

  Roedig, C ^a   Sesana, A ^a   Dotti, M ^b   Cuadra, J ^c   Amaro Seoane, P ^a,d   Haardt, F ^e  

^a ALBERT EINSTEIN INSTITUT   (Germany)

^b UNIVERSITY OF MILANO BICOCCA   (Italy)

^c PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^d UNIVERSITAT AUTÒNOMA DE BARCELONA   (Spain)

^e UNIVERSITY OF INSUBRIA   (Italy)

Author keywords

Accretion accretion disks; Black hole physics; Hydrodynamics; Methods: numerical

Indexed keywords

ACCRETION DISKS; ANGULAR MOMENTUM BUDGET; BLACK HOLE PHYSICS; BLACK HOLES; CO-ROTATION; COUPLED DYNAMICS; ECCENTRIC ORBITS; GAS STREAMS; GRAVITY TORQUE; LOW DENSITY; MASS RATIO; MASSIVE BLACK HOLES; MATERIAL FLOW; METHODS: NUMERICALS; NONRESONANT; SECULAR EVOLUTION; SEMIMAJOR AXIS; SMOOTHED PARTICLE HYDRODYNAMICS; SPECTRAL STRUCTURE; SPIRAL ARMS; THERMODYNAMICAL PROPERTIES; TIDAL TORQUE; TOTAL TORQUE;

ANGULAR MOMENTUM; HYDRODYNAMICS; MOMENTUM TRANSFER; NUMERICAL METHODS; STARS; THERMODYNAMICS; THREE DIMENSIONAL COMPUTER GRAPHICS; TORQUE;

GRAVITATION;

EID: 84866565576     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219986     Document Type: Article

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