Deriving pulsar sub-pulse widths from equivalent widths of integrated profiles

Details Deriving pulsar sub-pulse widths from equivalent widths of integrated profiles Deriving pulsar sub-pulse widths from equivalent widths of integrated profiles

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....66..463f&link_type=abstract

Astronomy and Astrophysics, vol. 66, no. 3, June 1978, p. 463, 464.

Astronomy and Astrophysics

Astronomy

1

Pulsars, Pulse Duration, Radio Astronomy, Spectral Line Width, Electromagnetic Pulses, Statistical Analysis

Scientific paper

The sub-pulse widths of pulsars are found to be closely related to the
equivalent widths of integrated profiles for pulsars of types S and C.
Conversion factors are derived which may enable sub-pulse widths to be
found for pulsars which are too weak to allow measurement of individual
pulses.

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