A statistical analysis of the fine temporal structure of the pulsar PSR 0809+74

Details A statistical analysis of the fine temporal structure of the pulsar PSR 0809+74 A statistical analysis of the fine temporal structure of the pulsar PSR 0809+74

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58..771s&link_type=abstract

Astronomicheskii Zhurnal, vol. 58, July-Aug. 1981, p. 771-778. In Russian.

Other

9

Fine Structure, Pulsars, Pulse Duration, Statistical Analysis, Stellar Radiation, Microstructure, Neutron Stars, Relativistic Particles, Root-Mean-Square Errors

Scientific paper

A statistical analysis is carried out of the microstructure of the pulses from PSR 0809+74. Two types of microstructures are established, one with a characteristic scale less than 500 microseconds, the other with a millisecond scale (0.6-9 milliseconds). It is found that the microstructure is often periodic, the distribution of periods being either 'short' (between 50 and 350 microseconds) or 'long' (between 1 and 10 milliseconds). The distribution of scales and the periodicity of the microstructure are discussed.

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