Production and evolution of millisecond X-ray and radio pulsars ☆
作者： Frederick K. Lamb
DOI: 10.1016/J.ASR.2006.08.003
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摘要: Abstract Observations using the Rossi X-ray Timing Explorer ( RXTE ) have discovered dozens of accreting neutron stars with millisecond spin periods in low-mass binary star systems. Eighteen are pulsars powered by accretion or nuclear burning both. These magnetic fields strong enough for them to become rotation-powered (radio) when ceases. Few, if any, accretion- rates higher than 750 Hz. There is evidence that spin-up some limited spin-equilibrium whereas others halted ends. Further study will show whether were emission gravitational radiation.
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