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Finding Pulsar Emission Heights from Dual–Frequency Observations

Published online by Cambridge University Press:  12 April 2016

Leszek A. Nowakowski
Leszek A. Nowakowski*
Affiliation:
Department of Physics, University of Puerto Rico, MayagüezPR 00681

Abstract

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We present a method that allows to find the radial separation of regions emitting individual components of pulsar average profiles at two radio frequencies. It may also be used for single–frequency observations in pulsars that have intensity–dependent average profiles and/or mode–switching. Preliminary results for three radio pulsars are presented, obtained using average profiles from non-simultaneous observations.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 219 - 220
Copyright
Copyright © Astronomical Society of the Pacific 2000

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