The cm and mm Variability of the Blazar Radiant Flux
Abstract
The radiant flux density variability of the extragalactic source is studied for the 1974-2005 period at the frequencies of 4.8, 8, 14.5, 22 and 36 GHz. The components of about 3 and 30 years of the long-term flux variability can be explained by the nutational and precession motions in a close double black-hole system. The fast flux variability component is not directly connected with rotation of the central black hole.
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Вольвач А.Е. Переменность потока излучения блазара 1633+382 в сантиметровом и миллиметровом диапазонах длин волн / А.Е. Вольвач, Х.Д. Аллер, М.Ф. Аллер // Радиофизика и радиоастрономия. — 2005. — Т. 10, № 4. — С. 377-385.
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