The Pulsar-Powered Nebula in G322.5-0.1

Details The Pulsar-Powered Nebula in G322.5-0.1 The Pulsar-Powered Nebula in G322.5-0.1

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop..846g&link_type=abstract

Chandra Proposal ID #03500310

Physics

Chandra Proposal Id #03500310

Scientific paper

The current small sample of young pulsars shows a wide range of properties. There is thus considerable motivation to discover new sources, both to identify unusual and interesting pulsars for further study, and to establish the properties of the overall population. Motivated by these issues, we here propose ACIS observations of the pulsar-powered nebula in the supernova remnant G322.5-0.1. We aim both to detect the central powering source and to use the nebular morphology to probe the properties of the pulsar's relativistic wind.

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