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Recycling Pulsars: spins, masses and ages
2012
Proceedings of the International Astronomical Union
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Although the first millisecond pulsars (MSPs) were discovered 30 years ago we still do not understand all details of their formation process. Here, we present new results from Tauris, Langer & Kramer (2012) on the recycling scenario leading to radio MSPs with helium or carbon-oxygen white dwarf companions via evolution of low- and intermediate mass X-ray binaries (LMXBs, IMXBs). We discuss the location of the spin-up line in the (P,Pdot)-diagram and estimate the amount of accreted mass needed
doi:10.1017/s1743921312023393
fatcat:iugisymoindljk6hjmcr3wq6zu