The 2.5-year Period in the Optical Variability of 3C 66A (Poster)

Details The 2.5-year Period in the Optical Variability of 3C 66A (Poster) The 2.5-year Period in the Optical Variability of 3C 66A (Poster)

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003heba.conf..205b&link_type=abstract

High Energy Blazar Astronomy, ASP Conference Proceedings, Vol. 299, held 17-21 June 2002 at Tuorla Observatory, Piikkio, Finland

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We analysed the optical light curve of the blazar 3C 66A which was cardinally improved by our extensive data set (1974-1991). Strong evidence for a 2.5-year period was found for the time interval of moderate activity of the object (1972-1992). The predictions made using this period are also in good agreement with the light variations in the time scale of months observed during the bright state (1993-1997).

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