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Blazars – INTEGRAL and Supermassive Black Hole Binaries

Published online by Cambridge University Press:  12 May 2006

R. Hudec ,
F. Munz ,
M. Basta  and
P. Kubanek
R. Hudec
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ–251 65 Ondrejov, Czech Republic email: rhudec@asu.cas.cz
F. Munz
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ–251 65 Ondrejov, Czech Republic email: rhudec@asu.cas.cz
M. Basta
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ–251 65 Ondrejov, Czech Republic email: rhudec@asu.cas.cz
P. Kubanek
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ–251 65 Ondrejov, Czech Republic email: rhudec@asu.cas.cz ISDC, Versoix, Switzerland
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Abstract

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We refer on analysis of the ESA INTEGRAL satellite data for blazars, promising sources to be observed during their active states. We further refer on searches for and analysis of supermassive binary black holes requiring very long time intervals (50 years and more) provided by digitised astronomical plates.

Keywords

Active Galactic NucleiBlazarsINTEGRAL
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S230: Populations of High Energy Sources in Galaxies , August 2005 , pp. 237 - 238
Copyright
2006 International Astronomical Union