Yi, InsuGrindlay, Jonathan E.2019-09-251998Yi, Insu, and Jonathan E. Grindlay. 1998. “Spin‐up of Low‐Luminosity, Low‐Mass X‐Ray Binaries.” The Astrophysical Journal 505 (2): 828–34. https://doi.org/10.1086/306193.0004-637X1538-4357http://nrs.harvard.edu/urn-3:HUL.InstRepos:41399835We examine the spin-up of low;luminosity, low-mass X-ray binaries (LMXBs) to millisecond pulsars (MSPs). In the conventional spin-up model of the Ghosh & Lamb type, where the stellar magnetic field interacts with the Keplerian accretion disk, MSPs could be produced from LMXBs if the magnetic field B* less than or similar to 10(8)((M) over dot/10(16) g s(-1)) G, where (M) over dot is the mass accretion rate. However, for (M) over dot < (M) over doten-USSpin‐up of Low‐Luminosity, Low‐Mass X‐Ray BinariesJournal Article2019-09-2510.1086/306193