The drifting subpulses of PSR 0148–06

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 h...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 1985-05, Vol.214 (1), p.47P-52P
Main Authors: Biggs, J. D., Hamilton, P. A., McCulloch, P. M., Manchester, R. N.
Format: Article
Language:English
Subjects:
Astronomy
Earth, ocean, space
Exact sciences and technology
Late stages of stellar evolution (including black holes)
Neutron stars
Stars
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Description
Summary: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.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/214.1.47P