@inproceedings{da5c98956a6248d9977df8718abd9ea3,
title = "The slow X-ray pulsar SXP 1062 and associated supernova remnant in the Wing of the Small Magellanic Cloud",
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.",
keywords = "Be, X-rays: binaries, pulsars: individual (SXP 1062), stars: emission-line",
author = "Oskinova, {L. M.} and Guerrero, {M. A.} and V. H{\'e}nault-Brunet and W. Sun and Chu, {Y. H.} and C. Evans and Gallagher, {J. S.} and Gruendl, {R. A.} and J. Reyes-Iturbide",
year = "2012",
month = aug,
doi = "10.1017/S1743921312024519",
language = "English (US)",
isbn = "9781107033801",
series = "Proceedings of the International Astronomical Union",
number = "S291",
pages = "459--461",
editor = "{Van Leeuwen}, Joeri",
booktitle = "Neutron Stars and Pulsars",
edition = "S291",
}