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Magnetic Models of Pulsars and Rotating Neutron Stars

Nature volume 222, pages 230–231 (1969)Cite this article

Abstract

The authors describe how magnetic models of pulsars can account for the narrowness of the beam of radiation.

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Authors and Affiliations

  1. P. N. Lebedev Physical Institute, Academy of Sciences, Moscow

    V. L. GINZBURG & V. V. ZAITSEV

Authors
  1. V. L. GINZBURG
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  2. V. V. ZAITSEV
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GINZBURG, V., ZAITSEV, V. Magnetic Models of Pulsars and Rotating Neutron Stars. Nature 222, 230–231 (1969). https://doi.org/10.1038/222230a0

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