Abstract
The results of multicolor observations of the blazar 3C 66A, obtained in the course of the project OJ-94, are analyzed. It is established that the energy distribution of the variable source in the optical and IR ranges can be represented, on the average, by a power law: Fν ∝ ν-0.92. Since the blazar's emission is strongly polarized, there is no doubt of the synchrotron nature of the variable source responsible for the blazar's activity.
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Hagen-Thorn, V.A., Hagen-Thorn, A.V., Jorstad, S.G. et al. Analysis of Multicolor Observations of 3C 66A in 1993-1998. Astrophysics 44, 283–291 (2001). https://doi.org/10.1023/A:1012809409416
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DOI: https://doi.org/10.1023/A:1012809409416