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Characteristics of Subpulses of Pulsar CP 1133

Nature Physical Science volume 235, pages 167–168 (1972)Cite this article

Abstract

WE have compared the amplitude and polarization characteristics of the two subpulses in the radio emission from pulsar CP 1133. The subpulses are designated I and II according to their time of arrival. The drift of subpulses in the pulse “window” is not observed for this pulsar as in the case of pulsar CP 0808, for example, where the “drift” is seen distinctly1.

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Authors and Affiliations

  1. P. N. Lebedev Physical Institute, Moscow

    YU. I. ALEKSEEV, V. V. VITKEVICH & V. M. MALOFEEV

Authors
  1. YU. I. ALEKSEEV
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  2. V. V. VITKEVICH
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  3. V. M. MALOFEEV
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ALEKSEEV, Y., VITKEVICH, V. & MALOFEEV, V. Characteristics of Subpulses of Pulsar CP 1133. Nature Physical Science 235, 167–168 (1972). https://doi.org/10.1038/physci235167b0

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