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

Oskinova, LM, Guerrero, MA, Hénault-Brunet, V, Sun, W, Chu, YH, Evans, C, Gallagher, JS, Gruendl, RA and Reyes-Iturbide, J (2012) The slow X-ray pulsar SXP 1062 and associated supernova remnant in the Wing of the Small Magellanic Cloud Proceedings of the International Astronomical Union, 8 (S291). pp. 459-461.

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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. © 2013 International Astronomical Union.

Item Type: Article
Authors :
NameEmailORCID
Oskinova, LMUNSPECIFIEDUNSPECIFIED
Guerrero, MAUNSPECIFIEDUNSPECIFIED
Hénault-Brunet, VUNSPECIFIEDUNSPECIFIED
Sun, WUNSPECIFIEDUNSPECIFIED
Chu, YHUNSPECIFIEDUNSPECIFIED
Evans, CUNSPECIFIEDUNSPECIFIED
Gallagher, JSUNSPECIFIEDUNSPECIFIED
Gruendl, RAUNSPECIFIEDUNSPECIFIED
Reyes-Iturbide, JUNSPECIFIEDUNSPECIFIED
Date : 1 August 2012
Identification Number : 10.1017/S1743921312024519
Depositing User : Symplectic Elements
Date Deposited : 17 May 2017 12:54
Last Modified : 17 May 2017 12:54
URI: http://epubs.surrey.ac.uk/id/eprint/837172

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