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Rotating Neutron Stars, Pulsars and Supernova Remnants

Naturevolume 219, pages145–146 (1968)Cite this article

Abstract

I SHALL discuss here some problems connected with theories linking the pulsars to the rotation of neutron stars (ref. 1 and a preprint by L. Woltjer). Because neutron stars can be formed during a supernova explosion, their rotation could be coupled with the surrounding gaseous remnant2,3: the following considerations will therefore also refer to the problem of the activity observed in the Crab Nebula and similar objects.

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References

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Author notes

  1. F. PACINI: On leave from Laboratorio d'Astrofisica, Frascati, Italy.

Authors and Affiliations

  1. Center for Radiophysics and Space Research, Cornell University, Ithaca, New York

    F. PACINI

Authors
  1. F. PACINI

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