Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/78
Title: Flux density evolution of the sources 3C273, 3C279 and 3C454.3 at the frequencies 102 MHz–36.8 GHz
Authors: Volvach, A. E.
Volvach, L. N.
Larionov, M. G.
Aller, H. D.
Aller, M. F.
Yurovskiy, Yu. Yu.
Riabov, Mykhailo I.
Citation: Astronomical & Astrophysical Transactions The Journal of the Eurasian Astronomical Society
Issue Date: 2007
Editors: Madrid : Consejo Superior de Investigaciones Científicas, Instituto Miguel Asín,
Keywords: Flux variations
Non-stationary extragalactic radio sources
Binary black holes
Series/Report no.: Vol. 25, Nos. 5–6, October–December 2006, 385–391
Abstract: The results of long-term monitoring of the sources 3C273, 3C279 and 3C454.3 at 102 MHz–36.8 GHz are presented. Numerical analysis of irregular temporal rows of the integral fluxes allowed us to detect the quasiperiodic constituents of the emission flux variations. The analysis of the parameters of binary black holes in the central regions of non-stationary objects demonstrates that these super-massive objects have an insignificant variation between the sizes of the orbits of partners, and that they are in the stage of evolution different from the time of merging by a period of less than 104 years.
URI: http://dspace.onu.edu.ua:8080/handle/123456789/78
ISSN: 1055-6796 print
1476-3540 online
Other Identifiers: DOI: 10.1080/10556790601135059
Appears in Collections:Статті та доповіді ФМФІТ

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