Published November 9, 1968
| public
Journal Article
Search for High Energy Gamma-rays from CP 1133
Chicago
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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.Additional details
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- CaltechAUTHORS:20151224-092941240
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