Articles written in Journal of Astrophysics and Astronomy
Volume 35 Issue 3 September 2014 pp 285-287 Posters
All the data of the blazar 3C446 at 8, 4.8, 14 and 22 GHz, presented in publications from 1977 to 2006, have been compiled to generate light curves. The light curves show violent activity of 3C446. Using Period04 analysis method, we have found that there is a period of 7.2 yr, which is consistent with the results that we found using wavelet analysis method. We get the instability region as 𝑟 = 123.83𝑟𝑔.
Volume 40 | Issue 6
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