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- W1534895571 abstract "Although most of the proposed equations of state predict minimum spin periods well below one millisecond if more than about 0.3 solar masses are accreted onto a low magnetized neutron star through a Keplerian accretion disc, the spin periods of the recently discovered accreting millisecond pulsars all cluster in the quite narrow range between 1.7 and 5.4 ms; these spin periods are uncomfortably higher than the theoretical predictions. We propose and discuss here the possibility that emission due to a magneto‐dipole rotator is relevant even during the accretion phase in fast‐spinning neutron stars; this mechanism is able to explain the quite long spin periods observed in both low mass X‐ray binaries and millisecond radio pulsars." @default.
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- W1534895571 date "2005-01-01" @default.
- W1534895571 modified "2023-09-24" @default.
- W1534895571 title "Accretion and Magneto-Dipole Emission in Fast-Rotating Neutron Stars: New Spin-Equilibrium Lines" @default.
- W1534895571 doi "https://doi.org/10.1063/1.2130220" @default.
- W1534895571 hasPublicationYear "2005" @default.
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