Quasi-periodicities of BL Lac Objects
arXiv:1801.06435 · doi:10.1051/0004-6361/201732550
Abstract
We review the reports of possible year-long quasi-periodicities of BL Lac objects in the -ray and optical bands, and present a homogeneous time analysis of the light curves of PKS2155304, PG1553+113, and BL Lac. Based on results from a survey covering the entire Fermi -ray sky we have estimated the fraction of possible quasi-periodic BL Lac objects. We compared the cyclical behaviour in BL Lac objects with that derived from the search of possible optical periodicities in quasars, and find that at z1 the cosmic density of quasi-periodic BL Lac objects is larger than that of quasi-periodic quasars. If the BL Lac quasi-periodicities were due to a supermassive binary black hole (SBBH) scenario, there could be a tension with the upper limits on the gravitational wave background measured by the pulsar timing array. The argument clearly indicates the difficulties of generally associating quasi-periodicities of BL Lac objects with SBBHs.
arXiv commentIn publication on A&A, 6 pages, 4 figure (11 plots). Minor corrections added
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