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Scientific paper
Jan 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...300..540d&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 300, Jan. 15, 1986, p. 540-550. Research supported by the Alfred P. Sloan F
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35
Null Zones, Pulsars, Stellar Radiation, Amplitude Distribution Analysis, Drift Rate, Pair Production, Radiant Flux Density
Scientific paper
The authors have studied the behavior of the drifting subpulses and nulling in PSR 1944+17 (P = 0.441 s), an object which allows a large number of null transitions to be examined, since 60% of the pulses are null pulses. No evidence for phase memory is found, but there are differences between the last pulse before a null and the other pulses in a burst. Two time scales are observed for the onset of a null. There is a decline of the pulse intensity for several pulse periods, followed by a rapid drop to the null state on a time scale 2 ms < τ < 30 ms. The implications of the measurements are briefly discussed in terms of polar cap models.
Cordes James M.
Deich William T. S.
Hankins Timothy H.
Rankin Joanna M.
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