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- W3100991551 abstract "We performed spectroscopic X-ray observations of the eastern and northern regions of the Cygnus Loop with the ASCA observatory. The X-ray surface brightness of these regions shows a complex structure in the ROSAT all-sky survey image. We carried out a spatially resolved analysis for both regions and found that kTe did not increase toward the center region, but showed inhomogeneous structures. Such variation cannot be explained by a blast-wave model propagating into a homogeneous interstellar medium. We thus investigated the interaction between a blast wave and an interstellar cloud. Two major emission mechanisms are plausible: a cloud evaporation model and a reflection-shock model. In both regions, only a reflection-shock model qualitatively explains our results. Our results suggest the existence of a large-scale interstellar cloud. We suppose that such a large-scale structure would be produced by a precursor." @default.
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- W3100991551 date "2001-05-10" @default.
- W3100991551 modified "2023-09-26" @default.
- W3100991551 title "Reflection‐shocked Gas in the Cygnus Loop Supernova Remnant" @default.
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- W3100991551 doi "https://doi.org/10.1086/320564" @default.
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