Electromagnetic counterparts of recoiling black holes: General relativistic simulations of non-Keplerian discs

Astronomy and Astrophysics

Volumn 523, Issue 1, 2010, Pages

  Zanotti, O ^a   Rezzolla, L ^a,b   Del Zanna, L ^c   Palenzuela, C ^a,d  

^a ALBERT EINSTEIN INSTITUT   (Germany)

^b LOUISIANA STATE UNIVERSITY   (United States)

^c UNIVERSITY OF FLORENCE   (Italy)

^d UNIVERSITY OF TORONTO   (Canada)

Author keywords

accretion, accretion disks; black hole physics; gravitational waves; relativistic processes

Indexed keywords

ACCRETION , ACCRETION DISKS; ACCRETION RATE; BINARY SYSTEMS; BLACK HOLE PHYSICS; BLACK HOLES; COOLING TIME; ELECTROMAGNETIC EMISSIONS; GRAVITATIONAL WAVES; HOLE SYSTEMS; PEAK VALUES; RADIATION TRANSFER; RECOIL VELOCITIES; RELATIVISTIC HYDRODYNAMICS; RELATIVISTIC PROCESSES; SHOCK DETECTORS; SUPERMASSIVE BLACK HOLES; TOTAL MASS;

DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); ELECTROMAGNETISM; GRAVITATIONAL EFFECTS; GRAVITY WAVES; LUMINANCE; MAGNETIC MATERIALS; MERGERS AND ACQUISITIONS; MERGING; RELATIVITY;

STARS;

EID: 78149448308     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014969     Document Type: Article

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