Rotating Neutron Stars, Pulsars and Supernova Remnants

Details Rotating Neutron Stars, Pulsars and Supernova Remnants Rotating Neutron Stars, Pulsars and Supernova Remnants

Jul 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968natur.219..145p&link_type=abstract

Nature, Volume 219, Issue 5150, pp. 145-146 (1968).

Physics

223

Scientific paper

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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