Binary pulsars before spin-up and PSR 1820 - 11

Details Binary pulsars before spin-up and PSR 1820 - 11 Binary pulsars before spin-up and PSR 1820 - 11

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.248p..21p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 248, Feb. 1, 1991, p. 21P-23P. Research supported by Al

Astronomy and Astrophysics

Astronomy

20

Pulsars, Stellar Evolution, X Ray Binaries, Radio Stars, Stellar Rotation

Scientific paper

It is argued that PSR 1820 - 11 may be a young pulsar, with a main-sequence companion, and that the system is the progenitor of a low-mass X-ray binary, rather than the descendant of one. If it is not, such a system should soon be found. The small number of antediluvian binary pulsars suggests that most, but not all, neutron stars have some torque decay after birth.

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