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Measuring the supermassive black hole parameters with space missions

Published online by Cambridge University Press:  01 August 2006

Alexander F. Zakharov
Alexander F. Zakharov*
Affiliation:
National Astronomical Observatories of Chinese Academy of Sciences, Beijing 100012, China ITEP, 25, B. Cheremushkinskaya st., Moscow 117259, Russia BLTP, JINR, Dubna, Russia email: zakharov@itep.ru
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Abstract

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Recent X-ray observations of microquasars and Seyfert galaxies reveal broad emission lines in their spectra, which can arise in the innermost parts of accretion disks. Recently Müller & Camenzind (2004) classified different types of spectral line shapes and described their origin. Zakharov (2006b) clarified their conclusions about an origin of doubled peaked and double horned line shapes in the framework of a radiating annulus model and discussed s possibility to evaluate black hole parameters analyzing spectral line shapes.

Keywords

Black holes – X-ray astronomy – supermassive black holes
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S238: Black Holes from Stars to Galaxies – Across the Range of Masses , August 2006 , pp. 475 - 476
Copyright
Copyright © International Astronomical Union 2007

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