Spin evolution in wind-fed X-ray binaries

Details Spin evolution in wind-fed X-ray binaries Spin evolution in wind-fed X-ray binaries

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.250p...3k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 250, May 15, 1991, p. 3P-5P.

Astronomy and Astrophysics

Astronomy

12

Angular Momentum, Neutron Stars, Stellar Evolution, Stellar Rotation, Stellar Winds, X Ray Binaries, Spin Dynamics, Stellar Mass Accretion

Scientific paper

Global angular momentum balance suggests that the neutron stars in
Be/X-ray binaries are not spinning in equilibrium. This requires an
X-ray lifetime of equal to or less than 100,000 yr, and suggests that
there are many 'dead' Be/X-ray binaries in the Galaxy. Some of these may
be turned up as millisecond radio pulsars with Be star companions.

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