Мощность гравитационного излучения блазара OJ 287
Journal: Izvestia. Ural Federal University Journal. Series 2. Humanities and Arts (Ural Federal University)
Year: 2020

Using a new model based on the consideration of close binary systems (CDS) of supermassive black holes (SMBHs), we obtained data for the OJ 287 blazar, which is necessary for finding the parameters of the OJ 287 gravitational radiation. We used the results of multi-frequency monitoring performed only in the radio band. The application of harmonic analyses of observational data allowed us to construct a model of CDS consisting of two SMBHs of comparable masses, which made it possible to find the