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Astrophysics > High Energy Astrophysical Phenomena

arXiv:1508.03115 (astro-ph)
[Submitted on 13 Aug 2015]

Title:Ultraluminous X-ray pulsar: accreting magnetar?

Authors:H. Tong
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Abstract:Magnetars are a special kind of neutron stars. There may also be accreting magnetars. From the studies of isolated magnetars, it is known that a neutron star with a strong dipole field only is not a magnetar. Super-slow X-ray pulsars may just be accreting high magnetic field neutron stars. The ultra-luminous X-ray pulsar NuSTAR J095551+6940.8 may be an accreting magnetar. It may be an accreting low magnetic field magnetar with multipole field of 10^14 G and dipole field of 10^12 G. This point of view is consistent with the study of isolated magnetars. An ultra-luminous X-ray pulsar phase in the binary evolution may result in massive millisecond pulsars.
Comments: 5 pages, 1 figure. submitted to the proceeding of SMFNS2015
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE)
Cite as: arXiv:1508.03115 [astro-ph.HE]
  (or arXiv:1508.03115v1 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.1508.03115

Submission history

From: Hao Tong [view email]
[v1] Thu, 13 Aug 2015 04:16:57 UTC (549 KB)
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