Direct observation of pulsar microstructure

Details Direct observation of pulsar microstructure Direct observation of pulsar microstructure

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976natur.260...25f&link_type=abstract

Nature, vol. 260, Mar. 4, 1976, p. 25-27.

Astronomy and Astrophysics

Astronomy

11

Fine Structure, Pulsars, Pulse Duration, Radio Astronomy, Time Signals, Autocorrelation, Bandwidth, Periodic Variations, Pulsed Radiation

Scientific paper

High-frequency observations of the pulsar PSR1133+16 have been obtained to investigate microstructure on a time scale of 14 microsec. Most observations were restricted to the first component of the double-pulse profile. The data for both components confirm the general features of the microstructure described by Hankins (1971; 1972; 1973). Autocorrelation functions of the strong pulses often exhibit the linear feature associated with microstructure, extending from near-zero lag to several hundred microseconds and followed by a broader feature associated with the subpulse width. Some pulses displayed quasi-periodic behavior within the pulse.

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