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Observations of the Millisecond Pulsar PSR 1855+09 At 102 MHz

Published online by Cambridge University Press:  27 September 2017

A. D. Kuz'min ,
Yu. I. Alekseev ,
K. A. Lapaev ,
B. Ya. Losovsky  and
A. A. Salnikov
A. D. Kuz'min
Affiliation:
Radio Astronomy Department, Lebedev Physical Institute
Yu. I. Alekseev
Affiliation:
Radio Astronomy Department, Lebedev Physical Institute
K. A. Lapaev
Affiliation:
Radio Astronomy Department, Lebedev Physical Institute
B. Ya. Losovsky
Affiliation:
Radio Astronomy Department, Lebedev Physical Institute
A. A. Salnikov
Affiliation:
Radio Astronomy Department, Lebedev Physical Institute

Abstract

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The study of millisecond pulsars is of great astrophysical interest. One may expect that the rotation effect on the structure of the magnetosphere should be very significant. In view of the short duration of the pulses they are very suitable for investigations of the interstellar medium; at least they hold the promise for the pulsar time scale.

Millisecond pulsars were discovered and have been studied on the basis of their radio-emission at decimeter wavelengths. At longer wavelengths scattering of the radio emission in the interstellar medium is the principal limitation of millisecond pulsar observations.

Type
Part V X-ray, γ-ray and millisecond pulsars
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 213
Copyright
Copyright © United States Naval Observatory 1992