Microstructure in the pulsar 0950+08 interpulse at radio wavelengths

Details Microstructure in the pulsar 0950+08 interpulse at radio wavelengths Microstructure in the pulsar 0950+08 interpulse at radio wavelengths

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...249..238h&link_type=abstract

Astrophysical Journal, Part 1, vol. 249, Oct. 1, 1981, p. 238-240. Research supported by the Alexander von Humboldt-Stiftung.

Astronomy and Astrophysics

Astronomy

6

Pulsars, Pulse Duration, Radio Astronomy, Autocorrelation, Data Smoothing, High Resolution, Periodic Variations, Temporal Resolution

Scientific paper

High time resolution measurements of the PSR 0950+08 interpulse intensity are made. It is found that the interpulse microstructure is similar to the main pulse microstructure, which implies that the emission mechanisms for the two regions must be similar. The characteristic microstructure time scale of 85 microseconds obtained from autocorrelation analysis compares with 130 microseconds obtained for the main pulse.

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