dc.contributor.author |
Tsygankov S. |
|
dc.contributor.author |
Mushtukov A. |
|
dc.contributor.author |
Suleimanov V. |
|
dc.contributor.author |
Poutanen J. |
|
dc.date.accessioned |
2018-09-19T21:57:29Z |
|
dc.date.available |
2018-09-19T21:57:29Z |
|
dc.date.issued |
2016 |
|
dc.identifier.issn |
0035-8711 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/144529 |
|
dc.description.abstract |
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.We present here the first convincing observational manifestation of a Magnetar-Like magnetic field in an accreting neutron star in binary System-The first pulsating ultraluminous X-Ray source X-2 in the galaxy M82. Using the Chandra X-Ray observatory data, we show that the source exhibit the bimodal distribution of the luminosity with Twowell-Defined peaks separated by a factor of 40. This behaviour can be interpreted as the action of the 'propeller regime' of accretion. The onset of the propeller in a 1.37 s pulsar at luminosity of ∼1040 erg s-1 implies the dipole component of the neutron star magnetic field of ∼1014 G. |
|
dc.relation.ispartofseries |
Monthly Notices of the Royal Astronomical Society |
|
dc.subject |
Accretion |
|
dc.subject |
Accretion Discs-Magnetic Fields-Stars |
|
dc.subject |
Binaries |
|
dc.subject |
Individual |
|
dc.subject |
M82 X-2-Stars |
|
dc.subject |
Magnetars-X-Rays |
|
dc.title |
Propeller effect in action in the ultraluminous accreting magnetar M82 X-2 |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
1 |
|
dc.relation.ispartofseries-volume |
457 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
1101 |
|
dc.source.id |
SCOPUS00358711-2016-457-1-SID84961627497 |
|