Very High Energy Observations of Pulsars

Details Very High Energy Observations of Pulsars Very High Energy Observations of Pulsars

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.6806s&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #68.06; Bulletin of the American Astronomical Society, Vol. 30, p.922

Astronomy and Astrophysics

Astrophysics

Scientific paper

The pursuit of Very High Energy (VHE) astrophysics (E>= 100 GeV) has resulted in the discovery of seven sources, of which three are associated with young spin-powered pulsars, namely, Crab Nebula, Vela pulsar and PSR B1706-44. We report here on the results of the periodic analysis on pulsars, in the VHE energy range, observed with the 10m gamma ray telescope at Whipple Observatory located on Mt. Hopkins, Arizona.

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