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- W3100552454 abstract "We have re-analysed the ASCA X-ray spectrum of the bright symbiotic star CH Cyg, which exhibits apparently distinct hard and soft X-ray components. Our analysis demonstrates that the soft X-ray emission can be interpreted as scattering of the hard X-ray component in a photoionized medium surrounding the white dwarf. This is in contrast to previous analyses in which the soft X-ray emission was fitted separately and assumed to arise independently of the hard X-ray component. We note the striking similarity between the X-ray spectra of CH Cyg and Seyfert 2 galaxies, which are also believed to exhibit scattering in a photoionized medium." @default.
- W3100552454 created "2020-11-23" @default.
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- W3100552454 date "2006-11-11" @default.
- W3100552454 modified "2023-09-27" @default.
- W3100552454 title "A new interpretation of the remarkable X-ray spectrum of the symbiotic star CH Cyg" @default.
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- W3100552454 doi "https://doi.org/10.1111/j.1365-2966.2006.10959.x" @default.
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