Search for High Energy Gamma-rays from CP 1133

Creators: Charman, W. N.; Jelley, J. V.; Orman, P. R.; Drever, R. W. P.; McBreen, B.

Abstract

Several proposed models for pulsars, involving shock waves and high magnetic fields, suggest the possibility that high energy γ-rays may be emitted by such objects. We have therefore attempted to detect high energy (~ 10^(14) eV), neutral cosmic rays from CP 1133, using the atmospheric Cherenkov technique.

Additional Information

© 1968 Nature Publishing Group. Received October 1, 1968. We arc grateful to Mr F. Pryce, of the Electronics Division at AERE, for setting up the electronics, and the staff of Jodrell Bank, who kindly provided advance information on the revised period of the source.

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Resource type: Journal Article
Publisher: Nature Publishing Group
Published in: Nature, 220(5167), 565-566, ISSN: 0028-0836.

Created:: August 19, 2023
Modified:: October 25, 2023