A model for the millisecond pulsar PSR 1937 + 214

Details A model for the millisecond pulsar PSR 1937 + 214 A model for the millisecond pulsar PSR 1937 + 214

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..98..201k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 98, no. 1, Jan. 1984, p. 201, 202.

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Binary Stars, Pulsars, Stellar Models, Angular Momentum, Momentum Transfer, Neutron Stars, Stellar Mass Accretion

Scientific paper

The authors suggest a model for the millisecond pulsar PSR 1937+214, according to which the immediate progenitor of the pulsar was a binary consisting of two neutron stars of unequal mass. The heavier neutron star was spun up by the transfer of angular momentum from the orbit, and the lighter neutron star was tidally disrupted, leaving behind a millisecond pulsar.

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