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The 1000 GeV gamma rays from ms pulsarsThe detection of 1000 GeV gamma-rays with the characteristic 6.1 ms periodicity of the radio pulsar PSR 1953 +29 is reported. This result, significant at the 5.4 beta level, provides the first direct evidence for the association of the 6 ms radio pulsar PSR1953+29 with the gamma-ray source 2CG065+0. Extensive observations of the 1.5 ms pulsar PSR 1937 are also reported.
Document ID
19850025635
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Chadwick, P. M. (Durham Univ.)
Dowthwaite, J. C. (Durham Univ.)
Kirkman, I. W. (Durham Univ.)
Mccomb, T. J. L. (Durham Univ.)
Orford, K. J. (Durham Univ.)
Turver, K. E. (Durham Univ.)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 1
Subject Category
Space Radiation
Report/Patent Number
OG-2.3-12
Accession Number
85N33948
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850025589Collected WorksNinteenth International Cosmic Ray Conference. OG Sessions, Volume 1
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