Timing of Young Pulsars

Details Timing of Young Pulsars Timing of Young Pulsars

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..124m&link_type=abstract

ATNF proposal P262, Semester: April, 2006

Physics

Stellar, Galactic, Parkes

Scientific paper

Young pulsars are of interest in several different ways: they are sometimes associated with supernova remnants, they sometimes have high-energy (optical, X-ray, gamma-ray) pulsed emission, and they usually have significant period variations and often suffer glitches. We propose frequent monitoring of the period of about 35 mostly young pulsars to provide a database for high-energy, ATCA and LBA observations of pulsars and to investigate variations in their period.

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