Analysis of Multicolor Observations of 3C 66A in 1993-1998

Details Analysis of Multicolor Observations of 3C 66A in 1993-1998 Analysis of Multicolor Observations of 3C 66A in 1993-1998

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap.....44..283h&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 44, Issue 3, p. 283-291 (2001).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

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: F -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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