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- W1967183507 abstract "Abstract Observational and theoretical evidence points to the existence of an unusually high magnetic field on GX 1+4. The pulsar is thus an ideal laboratory for studying two-photon cyclotron emission, an important source of photons of frequency significantly less than the cyclotron frequency in X-ray pulsars. Low-frequency approximations to the two-photon cyclotron emission transition probabilities are derived. These are used to calculate the theoretical opening angle of the double-humped pulse shape predicted by the two-photon cyclotron emission model. The theoretical pulse shape, incorporating the effects of gravitational light bending, is compared with observations of GX 1+4. Observed light curves have opening angles consistent with the theoretically predicted maximum value." @default.
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- W1967183507 date "1998-01-01" @default.
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- W1967183507 title "Investigating Pulse Morphology in GX 1+4" @default.
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- W1967183507 doi "https://doi.org/10.1071/as98217" @default.
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