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- W3135432007 abstract "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 power of gravitational radiation coming from OJ 287, variations in the orbit of the double SMDS, and to consider the possibility of experimentally determining changes in these parameters in the system. Variants of radiation of electromagnetic and gravitational waves coming from OJ 287 in various states of object activity are considered." @default.
- W3135432007 created "2021-03-15" @default.
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- W3135432007 date "2020-01-01" @default.
- W3135432007 modified "2023-10-16" @default.
- W3135432007 title "The gravitational radiation power of the blazar OJ 287" @default.
- W3135432007 doi "https://doi.org/10.15826/urej.2020.4.4.003" @default.
- W3135432007 hasPublicationYear "2020" @default.
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