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dc.contributor.author | Bychkova V.S. | |
dc.contributor.author | Kardashev N.S. | |
dc.contributor.author | Maslennikov K.L. | |
dc.contributor.author | Plokhotnichenko V.L. | |
dc.contributor.author | Beskin G.M. | |
dc.contributor.author | Karpov S.V. | |
dc.date.accessioned | 2021-02-25T20:37:15Z | |
dc.date.available | 2021-02-25T20:37:15Z | |
dc.date.issued | 2020 | |
dc.identifier.issn | 1063-7729 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/162060 | |
dc.description.abstract | © 2020, Pleiades Publishing, Ltd. Abstract—: The results of polarimetric observations of blazar S5 0716+714, carried out with the 6-meter BTA telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences, are presented. The polarized emission microvariability of blazar S5 0716+714 was observed in the R band with an initial time resolution of 3–5 seconds. Exposures were integrated at 1-minute intervals with a total observation time of several hours over two nights. Microvariability of the polarization degree with amplitude of 3–4% was detected during 7–11 minutes and flux oscillations within 9–10% during 25 minutes. A partial synchronism of the flux oscillations and the polarization degree of this blazar was found. Possible interpretations of the detected microvariability are briefly described. | |
dc.relation.ispartofseries | Astronomy Reports | |
dc.title | Rapid Polarized Emission Variability of Blazar S5 0716+714 in Optical Range | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 6 | |
dc.relation.ispartofseries-volume | 64 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 533 | |
dc.source.id | SCOPUS10637729-2020-64-6-SID85086572641 |