A possible reason for the peculiarity of the pulsar in the Crab nebula

Details A possible reason for the peculiarity of the pulsar in the Crab nebula A possible reason for the peculiarity of the pulsar in the Crab nebula

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..121b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Mar. 1977, p. 121-123. In Russian.

Astronomy and Astrophysics

Astrophysics

1

Crab Nebula, Pulsars, Stellar Mass Ejection, Astrophysics, Electric Field Strength, Helium, Surface Layers

Scientific paper

It is suggested that the peculiarity (i.e., the all-wave nature) of the
pulsar in the Crab nebula may be interpreted in terms of the outflow of
helium from the surface layer under the action of an ultrastrong
electric field. It is shown that this pulsar is presently in a state of
relaxation toward a state characteristic of other pulsars.

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