Search for TeV Emission from Pulsars with the Whipple Atmospheric

Details Search for TeV Emission from Pulsars with the Whipple Atmospheric Search for TeV Emission from Pulsars with the Whipple Atmospheric

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....3..523h&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

In systems containing pulsars, one may expect sufficient particle acceleration to produce extremely energetic photons. Reports of very high energy emission from such systems (Crab Nebula, PSR B1706-44, Vela, Centaurus X-3) have sparked recent interest. We present results from a search for very high energy photons (E 350 GeV) emitted from isolated pulsars and pulsars in binary systems utilizing the Whipple 10 m atmospheric Cherenkov telescope. Our results are compared with predictions of high energy emission from pulsar systems.

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