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 |
|