Spectral fitting of 2022 observations indicates the disk reaches 7-17 R_g from the neutron star at low inclination, with first reported type-II bursts attributed to magnetospheric gating.
V., Bhattacharya D., 2015, @doi [Monthly Notices of the Royal Astronomical Society] 10.1093/mnras/stv1542 , 452
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Application of an existing torque model to five AMXPs finds consistency with spin-up in outburst and spin-down in quiescence but cannot exclude gravitational wave contributions due to timing noise and bolometric uncertainties.
citing papers explorer
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On the assessment of the disk truncation and detection of type-II bursts from the accreting millisecond X-ray Pulsar IGR J17062-6143
Spectral fitting of 2022 observations indicates the disk reaches 7-17 R_g from the neutron star at low inclination, with first reported type-II bursts attributed to magnetospheric gating.
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The Torques Acting on Accreting Millisecond X-Ray Pulsars in the Outburst and Quiescent States, and During the Long-Term Evolution
Application of an existing torque model to five AMXPs finds consistency with spin-up in outburst and spin-down in quiescence but cannot exclude gravitational wave contributions due to timing noise and bolometric uncertainties.