The iron Kα lines as a tool for magnetic field estimations in non-flat accretion flows

New Astronomy

Volumn 9, Issue 8, 2004, Pages 663-677

  Zakharov, A F ^a,b,c   Ma, Z ^a   Bao, Y ^d  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b INSTITUTE FOR THEORETICAL AND EXPERIMENTAL PHYSICS   (Russian Federation)

^c LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^d SUN YAT SEN UNIVERSITY   (China)

Author keywords

Accretion; Black hole; Black hole physics; Line: profiles; Magnetic fields; Seyfert galaxies: MCG 6 30 15; X rays; Zeeman effect

Indexed keywords

ACCRETION; BLACK HOLE; BLACK HOLE PHYSICS; LINE; MCG-6-30-15; PROFILES; SEYFERT GALAXIES; ZEEMAN EFFECT;

ASTRONOMICAL SATELLITES; COMPUTER SIMULATION; DATABASE SYSTEMS; GALAXIES; MAGNETIC FIELDS; PARAMETER ESTIMATION; PHOTONS; X RAYS;

IRON;

EID: 4344711211     PISSN: 13841076     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.newast.2004.06.004     Document Type: Article

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