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Fluctuations in the 102-MHz pulse arrival time for four pulsars

Journal Article · · Sov. Astron. (Engl. Transl.); (United States)
OSTI ID:6052028
The pulse phase fluctuations of four pulsars have been monitored in a two-year observing program at 102.5-MHz frequency. For pulsars having P>1/sup s/, the frequency dependence of the phase residuals is tested to see whether the fluctuations might be attributable to emission-region displacements.
Research Organization:
Lebedev Physics Institute, USSR Academy of Sciences, Moscow
OSTI ID:
6052028
Journal Information:
Sov. Astron. (Engl. Transl.); (United States), Journal Name: Sov. Astron. (Engl. Transl.); (United States) Vol. 26:5; ISSN SAAJA
Country of Publication:
United States
Language:
English

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