期刊
ASTRONOMISCHE NACHRICHTEN
卷 336, 期 8-9, 页码 835-839出版社
WILEY-V C H VERLAG GMBH
DOI: 10.1002/asna.201512233
关键词
accretion; accretion disks; pulsars: general; stars: neutron
资金
- Xinjiang Bairen project
- West Light Foundation of CAS [LHXZ201201]
- 973 Program [2015CB857100]
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 during binary evolution may result in massive millisecond pulsars. ((c) 2015 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)
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