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Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the Small Magellanic Cloud
H. Klus, W. C. G. Ho, M. J. Coe +2
We report on the long-term average spin period, rate of change of spin period and X-ray luminosity during outbursts for 42 Be X-ray binary systems in the Small Magellanic Cloud. We…
XMM-Newton observation of the highly magnetised accreting pulsar Swift J045106.8-694803: Evidence of a hot thermal excess
E. S. Bartlett, M. J. Coe, W. C. G. Ho
Several persistent, low luminosity (L_X 10^{34} erg s^{-1}), long spin period (P>100 s) High Mass X-ray Binaries have been reported with blackbody components with temperatures >1 k…
Measuring the Cooling of the Neutron Star in Cassiopeia A with all Chandra X-ray Observatory Detectors
K. G. Elshamouty, C. O. Heinke, G. R. Sivakoff +5
The thermal evolution of young neutron stars (NSs) reflects the neutrino emission properties of their cores. Heinke et al. (2010) measured a 3.6+/-0.6% decay in the surface tempera…