Gravitational effects on the high energy emission of accreting black holes
T. SuebsuwongCentre d'Étude Spatiale des Rayonnements, CNRS-UPS, 9 avenue du Colonel Roche, 31028 Toulouse Cedex 4, France e-mail: [email protected]J. MalzacCentre d'Étude Spatiale des Rayonnements, CNRS-UPS, 9 avenue du Colonel Roche, 31028 Toulouse Cedex 4, France e-mail: [email protected]E. JourdainCentre d'Étude Spatiale des Rayonnements, CNRS-UPS, 9 avenue du Colonel Roche, 31028 Toulouse Cedex 4, France e-mail: [email protected]A. MarcowithCentre d'Étude Spatiale des Rayonnements, CNRS-UPS, 9 avenue du Colonel Roche, 31028 Toulouse Cedex 4, France e-mail: [email protected]
2006en
ABI
Аннотация
Context.We extend the investigation of general relativistic effects on the observed X-ray continuum of Kerr black holes in the context of the light bending model (Miniutti & Fabian 2004).
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