A pulsar too slow for its age

It is one of the slowest pulsars known, and its slowness seems incompatible with its age


SXP 1062 Pulsar and its remanent

V. Hénault-Brunet, L. M. Oskinova, M. A. Guerrero, W. Sun, Y.-H. Chu, C. J. Evans, J. S. Gallagher III, R. A. Gruendl, J. Reyes-Iturbide. Discovery of a Be/X-ray pulsar binary and associated supernova remnant in the Wing of the Small Magellanic Cloud. Monthly Notices of the Royal Astronomical Society. DOI: 10.1111/j.1745-3933.2011.01183.x



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Martín Guerrero, mar[at]iaa.es 958230622, 622233836