Role of emission angular directionality in spin determination of accreting black holes with a broad iron line

Astronomy and Astrophysics

Volumn 507, Issue 1, 2009, Pages 1-17

  Svoboda, J ^a   Dovciak M ^a   Goosmann, R ^a   Karas, V ^a  

^a ASTRONOMICAL INSTITUTE   (Czech Republic)

Author keywords

Accretion, accretion discs; Black hole physics; Galaxies: active; X rays: binaries

Indexed keywords

ACCRETION , ACCRETION DISCS; ACCRETION DISCS; BLACK HOLE PHYSICS; BLACK HOLES; CONFIDENCE LEVELS; DIRECTIONAL EMISSION; EMITTED PHOTONS; ENERGY BAND; FITTING PROCEDURE; GALAXIES : ACTIVE; GRAZING ANGLES; INNER REGION; ISOTROPIC DISTRIBUTIONS; LIMB DARKENING; LINE PROFILES; MARGINALLY STABLE ORBITS; MODEL DATA; PARAMETER SPACES; RADIATION TRANSFER; SEYFERT GALAXIES; SIMULATED DATA; SIMULATION RESULT; SPECTRAL BAND; X-RAY SPECTRA; XMM-NEWTON OBSERVATIONS;

ABSORPTION SPECTROSCOPY; GALAXIES; GRAVITATION; MULTIPHOTON PROCESSES; RELATIVITY; SIMULATORS; SOFTWARE PACKAGES; SPIN DYNAMICS; STARS; X RAY ANALYSIS; X RAY SPECTROGRAPHS; X RAYS;

ANGULAR DISTRIBUTION;

EID: 70449657201     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911941     Document Type: Article

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