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• W3101472939 abstract "We present the results of a spectral analysis of the central region of the mixed-morphology supernova remnant HB 9. A prior Ginga observation of this source detected a hard X-ray component above 4 keV and the origin of this particular X-ray component is still unknown. Our results demonstrate that the extracted X-ray spectra are best represented by a model consisting of a collisional ionization equilibrium plasma with a temperature of ~0.1-0.2 keV (interstellar matter component) and an ionizing plasma with a temperature of ~0.6-0.7 keV and an ionization timescale of >1 x 10^{11} cm^{-3} s (ejecta component). No significant X-ray emission was found in the central region above 4 keV. The recombining plasma model reported by a previous work does not explain our spectra." @default.
• W3101472939 created "2020-11-23" @default.
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• W3101472939 date "2020-05-25" @default.
• W3101472939 modified "2023-10-04" @default.
• W3101472939 title "X-ray emission from the mixed-morphology supernova remnant HB 9" @default.
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• W3101472939 doi "https://doi.org/10.1093/pasj/psaa042" @default.
• W3101472939 hasPublicationYear "2020" @default.
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