Long-term observations of galaxy 3C 66A

Monitoring of the active galaxy nucleus 3C 66A in the VHE γ-ray and analysis of data in X-rays and optical ranges over the period 1996–2009 were carried out. The nature of processes responsible for one or another type of radiation appeared to be very complicated since, at certain periods of time, an...

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Bibliographic Details
Published in:Bulletin of the Crimean Astrophysical Observatory 2011-06, Vol.107 (1), p.30-35
Main Authors: Zhovtan, A. V., Neshpor, Yu. I., Zhogolev, N. A., Nehai, E. M., Skiruta, Z. N., Fomin, V. P.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Astrophysics and Cosmology
Physics
Physics and Astronomy
Radiation
Stars & galaxies
X-rays
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Summary:Monitoring of the active galaxy nucleus 3C 66A in the VHE γ-ray and analysis of data in X-rays and optical ranges over the period 1996–2009 were carried out. The nature of processes responsible for one or another type of radiation appeared to be very complicated since, at certain periods of time, an either positive or negative correlation may be observed between different types of radiation. Period of radiation P = 365 days in the X-ray range was found.
ISSN:0190-2717
1934-7863
DOI:10.3103/S0190271711010189