Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..84..243o&link_type=abstract
Astrophysics and Space Science, vol. 84, no. 1, May 1982, p. 243-246.
Astronomy and Astrophysics
Astrophysics
1
Pulsars, Stellar Evolution, Stellar Models, Stellar Magnetic Fields, Stellar Rotation
Scientific paper
Depending on the evolutionary model adopted, the phenomenon of nulling is either intrinsic to all pulsars, occurring at a certain stage of their evolution, or peculiar to only a class of pulsars. The first model considered, involving the sudden ceasure of rotation and consequent abrupt death of pulsars, does not appear to explain the nulling phenomenon. A second model, in which evolution is partially discontinuous after field decay, is more plausible. It is concluded that detailed single-pulse observations of several pulsars are required before the origin of pulsar nulling can be established.
Akujor Chidi E.
Okeke P. N.
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