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 |
|