X-Ray Emission from Young Radio Pulsars Discovered in the Parkes Multibeam Survey

Details X-Ray Emission from Young Radio Pulsars Discovered in the Parkes Multibeam Survey X-Ray Emission from Young Radio Pulsars Discovered in the Parkes Multibeam Survey

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1209s&link_type=abstract

Chandra Proposal ID #04500372

Physics

Chandra Proposal Id #04500372

Scientific paper

The young (characteristic age = 10--100 kyr) pulsars represent a transition group from the very young pulsars, characterized by strong nonthermal radiation and bright synchrotron pulsar wind nebulae, to the middle aged pulsars, characterized by the thermal radiation. The investigation of these pulsars allows us to understand the transition from very young to middle-aged pulsars and constrain the parameters responsible for pulsar evolution, and potentially detect the PWN around these pulsars. Therefore, we propose to observe four young pulsars recently discovered in the Parkes Multibeam Pulsar Survey.

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