Secondary Periodicities in Pulsars

Physics

Scientific paper

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Scientific paper

PERIODIC intensity fluctuations in pulsars, first noted by Conklin et al.1 in CP 1919, have now been reported by a number of observers2-9. The present data support the earlier results. They also reveal a very pronounced modulation for CP 0834 which cannot be explained readily by current theories and give an upper limit for the stability of the secondary periodicity in the case of CP 1919.

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