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The Relation between Spin and Orbital Periods in HMXBs
Published online by Cambridge University Press: 26 May 2016
Abstract
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The relation between the spin period (Ps) and the orbital period (Po) in high-mass X-ray binaries (HMXBs) is investigated. In order for Be/X-ray binaries to locate above the critical line of observable X-ray emission due to accretion, it is necessary for an intermediate orbital eccentricity to be introduced. We suggest that some peculiar systems in the Po − Ps diagram are caused by their peculiar magnetic fields.
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- Part 6 X-Ray Binaries
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- Copyright © Astronomical Society of the Pacific 2003