NASA NTRS ยท 20090019024
Accreting X-ray Pulsars
Abstract
This presentation describes the behavior of matter in environments with extreme magnetic and gravitational fields, explains the instability/stability of accretion disks in certain systems, and discusses how emergent radiation affects accretion flow. Magnetic field measurements are obtained by measuring the lowest cyclotron absorption line energy, observing the cutoff of accretion due to centrifugal inhibition and measuring the spin-up rate at high luminosity.
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Wilson-Hodge, Colleen A.. 2009-01-05. Accreting X-ray Pulsars. https://ntrs.nasa.gov/citations/20090019024
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