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 |
|