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- W2017163150 abstract "We study the properties of pulsed component of hard (2–10 keV) x-ray emission from pulsars based on the new version of outer gap model we proposed previously [Astrophys. J. 604 (2004) 317]. On the frame of this outer gap model, we derive an expression of non-thermal pulsed x-ray luminosity of rotation-powered pulsars, and then apply it to the pulsars whose pulsed x-rays are detected by ASCA. Using the Kolmogorov–Smirnov test, we determine the model parameter. The present results indicate LXL1.15sd for these x-ray pulsars, which is consistent with the observed data." @default.
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- W2017163150 date "2005-03-23" @default.
- W2017163150 modified "2023-09-24" @default.
- W2017163150 title "X-Ray Emission from Rotation-Powered Pulsars" @default.
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- W2017163150 doi "https://doi.org/10.1088/0256-307x/22/4/067" @default.
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