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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 |