Long-term evolution of the neutron-star spin period of SXP 1062

DISCOVERY OF X-RAY EMISSION FROM YOUNG SUNS IN THE SMALL MAGELLANIC CLOUD

(2013) L. M. Oskinova et al.   ASTROPHYSICAL JOURNAL

COULD SXP 1062 BE AN ACCRETING MAGNETAR?

(2012) Lei Fu et al.   ASTROPHYSICAL JOURNAL

On the periodicities present in the optical light curves of Small Magellanic Cloud Be/X-ray binaries

(2012) A. J. Bird et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

SXP 1062, a young Be X-ray binary pulsar with long spin period

(2011) F. Haberl et al.   ASTRONOMY & ASTROPHYSICS

Be/X-ray binaries

(2011) Pablo Reig   ASTROPHYSICS AND SPACE SCIENCE

The first XMM-Newton slew survey catalogue: XMMSL1

(2008) R. D. Saxton et al.   ASTRONOMY & ASTROPHYSICS

XMM-Newton observations of the Small Magellanic Cloud: Be/X-ray binary pulsars active between October 2006 and June 2007

(2008) F. Haberl et al.   ASTRONOMY & ASTROPHYSICS

The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars

(2008) Sandro Mereghetti   ASTRONOMY AND ASTROPHYSICS REVIEW