X-ray Emission Properties Of Old Pulsars

Details X-ray Emission Properties Of Old Pulsars X-ray Emission Properties Of Old Pulsars

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0123b&link_type=abstract

American Astronomical Society, HEAD meeting #9, #1.23; Bulletin of the American Astronomical Society, Vol. 38, p.332

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Young and middle aged neutron stars, which emit strong pulsed non-thermal and/or surface hot-spot plus cooling emission, were studied reasonable well by previous X-ray observatories. In contrast, most old radio pulsars were too faint for a detailed examination of their X-ray emission and are clearly sources which required the sensitivity of Chandra and XMM-Newton. In my talk I will review recent results which suggest that the current picture of old pulsars emitting mostly thermal hot-spot emission is no longer in agreement with the observations. I further report on a study of the diffuse trail like emission components found in the vicinity of e.g. PSR 1929+10 and few other old pulsars.

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