The drifting subpulses of PSR 0148-06

Details The drifting subpulses of PSR 0148-06 The drifting subpulses of PSR 0148-06

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214p..47b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, June 1, 1985, p. 47P-52P.

Astronomy and Astrophysics

Astronomy

3

Electromagnetic Pulses, Pulsars, Radio Sources (Astronomy), Amplitude Modulation, Cross Correlation, Drift Rate, Pulse Duration, Radiant Flux Density

Scientific paper

Drifting subpulses have been detected at 645 MHz in observations of individual pulses from PSR 0148-06. The integrated pulse profile has two well-resolved components. Distinct drifting subpulses are visible in the earliest component whilst, in the later component, drifting is weak. Both components have a strong periodic amplitude modulation associated with the drifting subpulses.

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