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dc.contributor.author | Trushkin S. | |
dc.contributor.author | Nizhelskij N. | |
dc.contributor.author | Tsybulev P. | |
dc.contributor.author | Zhekanis G. | |
dc.date.accessioned | 2018-04-05T07:10:21Z | |
dc.date.available | 2018-04-05T07:10:21Z | |
dc.date.issued | 2017 | |
dc.identifier.uri | http://dspace.kpfu.ru/xmlui/handle/net/130393 | |
dc.description.abstract | © 2017 by the authors. We report on the radio properties of jets of the following microquasars, as determined from daily multi-frequency monitoring observations with the RATAN-600 radio telescope during 2010-2017: V404 Cyg, SS433, Cyg X-1, GRS1915+105 and LSI+61°303. We have detected many giant flares from SS433, a powerful flare from V404 Cyg in June 2015, an active state of Cyg X-1 in 2017 and fifty periodic flares from LSI+61°303. We describe the properties of massive ejections based on multi-band (radio, X-ray and γ-ray) studies. The general properties of the light curves are closely connected with the processes of jet formation in microquasars. | |
dc.subject | Black hole | |
dc.subject | Microquasars | |
dc.subject | Radio emission | |
dc.subject | Relativistic jets | |
dc.subject | Stars | |
dc.subject | Synchrotron radiation | |
dc.subject | X-ray binary | |
dc.subject | X-ray emission | |
dc.title | The jets of microquasars during giant flares and quiet state | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 4 | |
dc.relation.ispartofseries-volume | 5 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS-2017-5-4-SID85036655780 |