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Magnetic Models of Pulsars and Rotating Neutron Stars

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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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  • DOI: https://doi.org/10.1038/222230a0

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