Be/neutron star binaries - Orbital and spin periods

Details Be/neutron star binaries - Orbital and spin periods Be/neutron star binaries - Orbital and spin periods

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40..409c&link_type=abstract

(ESA, ESLAB Symposium on X-Ray Astronomy in the EXOSAT Era, 18th, The Hague, Netherlands, Nov. 5-9, 1984) Space Science Reviews

Astronomy and Astrophysics

Astronomy

9

B Stars, Binary Stars, Neutron Stars, Stellar Orbits, Stellar Rotation, Variable Stars, Correlation Coefficients, Eccentric Orbits, Spin Dynamics, Stellar Envelopes

Scientific paper

The spin periods of accreting neutron stars in binary systems with Be star primaries are shown to depend more strongly on periastron distance than apastron distance. This is interpreted as showing that neutron stars spin-up on shorter timescales than they spin-down. The pulse and orbital periods of V 0332+53 suggest that the optical counterpart of this source is a Be star.

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