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dc.contributor.author | Shibanov Y. | |
dc.contributor.author | Beskin G. | |
dc.contributor.author | Karpov S. | |
dc.contributor.author | Plokhotnichenko V. | |
dc.contributor.author | Zyuzin D. | |
dc.contributor.author | Kholtygin A. | |
dc.contributor.author | Sokolov V. | |
dc.contributor.author | Baryshev Y. | |
dc.date.accessioned | 2018-04-05T07:09:59Z | |
dc.date.available | 2018-04-05T07:09:59Z | |
dc.date.issued | 2017 | |
dc.identifier.issn | 1742-6588 | |
dc.identifier.uri | http://dspace.kpfu.ru/xmlui/handle/net/130116 | |
dc.description.abstract | © Published under licence by IOP Publishing Ltd. We briefly report first results of high time resolution optical multi-band panoramic photo-polarimetric observations of the eclipsing binary millisecond redback pulsar J1023+0038 obtained in February 2017 with the 6 m BTA telescope. The time resolution was varied from 10 to 120 ms depending on observational mode. Our data show that the pulsar still remained in the low-mass X-ray binary stage, characterised by rapid flaring at time scales of 10-100 s with amplitudes of 0.2-0.5 mag. We resolved a fine structure of the flares at time scales of 0.1-10 s. The polarimetry at the time scale of 0.1 s shows no polarization with an upper limit of 2%-4% for the linear polarisation degree in flaring and quiet stages, while at a 10 minute scale averaging it is about 1.5% at 3σ significance. We shortly outline implications of the results. | |
dc.relation.ispartofseries | Journal of Physics: Conference Series | |
dc.title | High time resolution multi-band photo-polarimetric observations of the binary millisecond redback pulsar J1023+0038 with the BTA | |
dc.type | Conference Paper | |
dc.relation.ispartofseries-issue | 1 | |
dc.relation.ispartofseries-volume | 932 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS17426588-2017-932-1-SID85039445230 |