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Results of Pulsar Timing Observations at 102.5 MHz

Published online by Cambridge University Press:  27 September 2017

T. V. Shabanova
T. V. Shabanova*
Affiliation:
Radio Astronomy Department, Lebedev Physical Institute

Abstract

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A program of pulse arrival time observations made at Pushchino during 1978-1986 is described. The period, period derivative and position derived from the full timing solutions were obtained for 16 pulsars. Comparison of our results with others obtained during 1970-1980 by different groups has shown that the parameters for a number of pulsars have suffered a significant change.

Type
Part II Evolution of the magnetic field
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 49 - 51
Copyright
Copyright © United States Naval Observatory 1992