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- W3100210332 abstract "CH Cygni is a symbiotic star consisting of an M giant and an accreting white dwarf, which is known to be a highly variable X-ray source with a complex, two-component, spectra. Here we report on two Suzaku observations of CH Cyg, taken in 2006 January and May, during which the system was seen to be in a soft X-ray bright, hard X-ray faint state. Based on the extraordinary strength of the 6.4 keV fluorescent Fe K-alpha line, we show that the hard X-rays observed with Suzaku are dominated by scattering." @default.
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- W3100210332 date "2007-01-30" @default.
- W3100210332 modified "2023-09-28" @default.
- W3100210332 title "An Apparent Hard X-Ray Decline of CH Cygni" @default.
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- W3100210332 doi "https://doi.org/10.1093/pasj/59.sp1.s177" @default.
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