Detection of a quasi-periodic oscillation in the optical light curve of the remarkable blazar AO 0235+164

ROY, A.; CHITNIS, V. R.; GUPTA, A. C.; WIITA, P. J.; ROMERO, G. E.; CELLONE, S. A.; CHATTERJEE, A.; COMBI, J. A.; RAITERI, C. M.; SARKAR, A.; VILLATA, M.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

WILEY-BLACKWELL PUBLISHING, INC

Lugar: Londres; Año: 2022 vol. 513 p. 5238 - 5244

0035-8711

We present a long term optical R band light-curve analysis of the gravitationally lensed blazar AO 0235+164 in the time span 1982?2019. Several methods of analysis lead to the result that there is a periodicity of ∼8.13 yr present in these data. In addition, each of these five major flares are apparently double-peaked, with the secondary peak following the primary one by ∼2 yr.Along with the well-known system, OJ 287, our finding constitutes one of the most secure cases of long-term quasi-periodic optical behaviour in a blazar ever found. A binary supermassive black hole system appears to provide a good explanation for these results.