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Theoretical X-ray line profiles from colliding wind binaries
Published online by Cambridge University Press: 26 May 2016
Abstract
We present theoretical X-ray line profiles calculated for a range of model colliding wind systems. In particular we have investigated how the line profiles vary with wind parameters. These profiles will be compared with high-resolution grating spectra of colliding wind binaries and will provide new insights into the structure of the X-ray emitting regions in such systems.
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- Part 1. Atmospheres of Massive Stars
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- Copyright © Astronomical Society of the Pacific 2003
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