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Search for High Energy Gamma-rays from CP 1133

Charman, W. N. and Jelley, J. V. and Orman, P. R. and Drever, R. W. P. and McBreen, B. (1968) Search for High Energy Gamma-rays from CP 1133. Nature, 220 (5167). pp. 565-566. ISSN 0028-0836. http://resolver.caltech.edu/CaltechAUTHORS:20151224-092941240

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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.


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http://dx.doi.org/10.1038/220565a0DOIArticle
http://www.nature.com/nature/journal/v220/n5167/abs/220565a0.htmlPublisherArticle
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.
Record Number:CaltechAUTHORS:20151224-092941240
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20151224-092941240
Official Citation:Search for High Energy Gamma-rays from CP 1133 565 W. N. CHARMAN, J. V. JELLEY, P. R. ORMAN, R. W. P. DREVER & B. MCBREEN doi:10.1038/220565a0
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:63222
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:24 Dec 2015 17:38
Last Modified:24 Dec 2015 17:38

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