Diversity in Neutron Stars: X-ray Observations of High-Magnetic-Field Radio Pulsars

Details Diversity in Neutron Stars: X-ray Observations of High-Magnetic-Field Radio Pulsars Diversity in Neutron Stars: X-ray Observations of High-Magnetic-Field Radio Pulsars

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011head...12.2603k&link_type=abstract

American Astronomical Society, HEAD meeting #12, #26.03

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Scientific paper

Young neutron stars show a surprising diversity in observational behavior. Many different `classes' of these objects are presently inferred, including rotation-powered pulsars, magnetars, CCOs, INSs, among others. In this presentation I review a critical group of neutron stars that sit at the juncture of multiple such classes: the high-magnetic field rotation-powered pulsars. Deep X-ray studies of multiple high-B sources have now been done, and have revealed possible evidence for
enhanced thermal emission, as predicted by models of magneto-thermal evolution. These observations will be described, and the evidence for enhanced cooling presented.

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