Searching for pulsars associated to recently detected Pulsar Wind Nebulae and X-ray point sources in Supernova Remnants

Details Searching for pulsars associated to recently detected Pulsar Wind Nebulae and X-ray point sources in Supernova Remnants Searching for pulsars associated to recently detected Pulsar Wind Nebulae and X-ray point sources in Supernova Remnants

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop..971b&link_type=abstract

ATNF proposal P589, Semester: April, 2007

Physics

Stellar, Galactic, Parkes

Scientific paper

Recent XMM observations of three shell type supernova remnants (SNRs), done by some of the proposers of this project, led to the discovery of new candidate pulsar wind nebulae and hard X-ray point sources, higly suggestive of the presence of an active radio pulsar in the remnants. We hence popose to observe the three X-ray point sources for a full transit (~9 hr each) to search for radio pulsations from young faint pulsars.

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