Role of magnetic fields during the stellar collapse and origin of binary pulsars

Details Role of magnetic fields during the stellar collapse and origin of binary pulsars Role of magnetic fields during the stellar collapse and origin of binary pulsars

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...126l..11p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 126, no. 2, Oct. 1983, p. L11, L12. Research supported by the Ministero della

Astronomy and Astrophysics

Astrophysics

9

Binary Stars, Gravitational Collapse, Pulsars, Stellar Magnetic Fields, Angular Momentum, Stellar Rotation

Scientific paper

The author suggests that pulsars originate with a stellar collapse whose
time scale is determined by the electromagnetic removal of angular
momentum. This may explain why binary pulsars generally have weak
magnetic fields and leads to the expectation of a large number of
binaries among very fast, weakly magnetized neutron stars.

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