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arXiv · 1210.5066

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

L. M. Oskinova·M. A. Guerrero·V. Henault-Brunet·W. Sun·Y. -H. Chu·C. Evans·J. S. Gallagher III·R. A. Gruendl·J. Reyes-Iturbide
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Abstract

SXP 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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L. M. Oskinova, M. A. Guerrero, V. Henault-Brunet, W. Sun, Y. -H. Chu, C. Evans, J. S. Gallagher III, R. A. Gruendl, J. Reyes-Iturbide. 2012-10-18. The slow X-ray pulsar SXP 1062 and associated supernova remnant in the Wing of the Small Magellanic Cloud. https://doi.org/10.1017/s1743921312024519

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