Search for Giant Pulses in High Edot Pulsars

Details Search for Giant Pulses in High Edot Pulsars Search for Giant Pulses in High Edot Pulsars

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aps..ses.hb003i&link_type=abstract

American Physical Society, 73rd Annual Meeting of the Southeastern Section of the APS, November 9-11, 2006, abstract #HB.003

Physics

Scientific paper

In order to investigate a possible correlation between the Edot of a pulsar and the presence of giant pulses, we made observations of pulsars J1930+1852, B1951+32 and J1913+1011 using the WAPP (Wideband Arecibo Pulsar Processor) at the Arecibo Observatory. We chose these pulsars because they possess high Edots, a characteristic shared by the Crab Pulsar, PSR B1937+21, PSR B0540-69 and B1821-24; four of the few currently known giant pulse emitters. Although no giant pulses were positively identified, PSR J1913+1011 showed enough possible evidence to warrant further research.

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