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Feeding Neutron Stars in High-Mass X-ray Binaries

Published online by Cambridge University Press:  21 February 2013

L. Fu ,
Z. Zhang  and
X.-D. Li
L. Fu
Affiliation:
Department of Astronomy and Key laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing 210093, China
Z. Zhang
Affiliation:
Department of Astronomy and Key laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing 210093, China
X.-D. Li
Affiliation:
Department of Astronomy and Key laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing 210093, China
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Abstract

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We suggest that the Be/X-ray binary SXP 1062 and the supergiant fast X-ray transient AX J1841.0-0536 belong to accreting magnetars and anti-magnetars, respectively.

Keywords

Stars: neutronX-rays: binaries: SXP 1062AX J1841.0-0536
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 129 - 132
Copyright
Copyright © International Astronomical Union 2013

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