Rotating Neutron Stars and Pulsar Emission

Details Rotating Neutron Stars and Pulsar Emission Rotating Neutron Stars and Pulsar Emission

Feb 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.221..624b&link_type=abstract

Nature, Volume 221, Issue 5181, pp. 624-626 (1969).

Physics

16

Scientific paper

The oblique rotator model of a neutron star can provide a mechanism to
transfer rotational energy into the circumstellar plasma, producing
periodic shock waves. This mechanism is also relevant to the activity
sometimes observed in supernovae remnants.

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