Journal
ASTROPHYSICAL JOURNAL
Volume 558, Issue 1, Pages 302-308Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/322469
Keywords
pulsars : general; pulsars : individual (B0823+26; B0950+08, B1133+16, 1937+21); stars : neutron
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The statistical properties of the radio emission from the pulsars B0823+26, B0950+08, B1133+16, and B1937+21 are studied using high time resolution observations taken at the Arecibo Observatory in Puerto Rico. Temporally coherent non-Gaussian emission has been detected in three of the four observed objects. This is the first time such a phenomenon has been observed. The results have been interpreted using a generalized shot noise model, and various basic physical quantities pertaining to the magnetospheric plasma have been estimated.
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