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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PACINI, F. Rotating Neutron Stars, Pulsars and Supernova Remnants. Nature 219, 145–146 (1968). https://doi.org/10.1038/219145a0
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DOI: https://doi.org/10.1038/219145a0
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