New SED fitting of ASKAP J1745-5051 using model atmospheres, corrected photometry, and added NIR data yields a 15,000 K WD plus 0.05 solar-mass sub-stellar donor at ~320 pc, suggesting a period-bouncer CV.
M., et al., 2009, @doi [Science] 10.1126/science.1172740 , https://ui.adsabs.harvard.edu/abs/2009Sci...324.1411A 324
2 Pith papers cite this work. Polarity classification is still indexing.
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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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The Long-Period Radio Transient and Cataclysmic Variable ASKAP J1745-5051: Evidence for a 15,000 K White Dwarf and a Sub-Stellar Donor
New SED fitting of ASKAP J1745-5051 using model atmospheres, corrected photometry, and added NIR data yields a 15,000 K WD plus 0.05 solar-mass sub-stellar donor at ~320 pc, suggesting a period-bouncer CV.
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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.