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

Published online by Cambridge University Press:  20 March 2013

L. M. Oskinova ,
M. A. Guerrero ,
V. Hénault-Brunet ,
W. Sun ,
Y.-H. Chu ,
C. Evans ,
J. S. Gallagher III ,
R. A. Gruendl  and
J. Reyes-Iturbide
L. M. Oskinova
Affiliation:
Institute for Physics and Astronomy, University of Potsdam, 14476 Potsdam, Germany, email: [email protected]
M. A. Guerrero
Affiliation:
Instituto de Astrofisica de Andalucia, IAA-CSIC, Granada, Spain
V. Hénault-Brunet
Affiliation:
Scottish Universities Physics Alliance (SUPA), Institute for Astronomy, University of Edinburgh, UK
W. Sun
Affiliation:
Department of Astronomy, Nanjing University, Nanjing, 210093 Jiangsu, China
Y.-H. Chu
Affiliation:
Department of Astronomy, University of Illinois, 1002 West Green St., Urbana, IL 61801, USA
C. Evans
Affiliation:
Scottish Universities Physics Alliance (SUPA), Institute for Astronomy, University of Edinburgh, UK
J. S. Gallagher III
Affiliation:
Department of Astronomy, University of Wisconsin-Madison, Madison, WI 53706, USA
R. A. Gruendl
Affiliation:
Department of Astronomy, University of Illinois, 1002 West Green St., Urbana, IL 61801, USA
J. Reyes-Iturbide
Affiliation:
Escuela Superior de Fisica y Matematicas, IPN, U.P. Adolfo López Mateos, C.P. 07738 D.F., Mexico
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Abstract

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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.

Keywords

stars: emission-lineBeX-rays: binariespulsars: individual (SXP 1062)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 459 - 461
Copyright
Copyright © International Astronomical Union 2013

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