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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S291(8), p. 459-461, 2012

DOI: 10.1017/s1743921312024519

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The slow X-ray pulsar SXP 1062 and associated supernova remnant in the Wing of the Small Magellanic Cloud

Journal article published in 2012 by L. M. Oskinova, M. A. Guerrero ORCID, V. Hénault-Brunet, W. Sun, Y.-H. Chu, C. Evans, J. S. Gallagher, R. A. Gruendl, J. Reyes-Iturbide
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractSXP 1062 is an exceptional case of a young neutron star in a wind-fed high-mass X-ray binary associated with a supernova remnant. A unique combination of measured spin period, its derivative, luminosity and young age makes this source a key probe for the physics of accretion and neutron star evolution. Theoretical models proposed to explain the properties of SXP 1062 shall be tested with new data.

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