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- W3099682755 abstract "We present X-ray equivalent width imaging of 3C 397 for Mg Heα, Si Heα, S Heα, and Fe Kα complex lines with Chandra and XMM-Newton observations. The images revealed that the heavier the element is, the smaller the extent of the element distribution is. The Mg emission is evidently enhanced in the southeastern blow-out region, well along the radio boundary there, and appears to partially envelope the eastern Fe knot. Two bilateral hat-like Si line-emitting structures are along the northern and southern borders, roughly symmetric with respect to the south-east-northwest elongation axis. An S line-emitting shell is located just inside the northern radio and IR shell, indicating a layer of reversely shocked sulphur in the ejecta. A few enhanced Fe features are basically aligned along the diagonal of the rectangular shape of the SNR, which implicates an early asymmetric SN explosion." @default.
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- W3099682755 date "2010-01-01" @default.
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- W3099682755 title "Spatial distribution of metal emissions in supernova remnant 3C 397 viewed with Chandra and XMM" @default.
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- W3099682755 doi "https://doi.org/10.1007/s11433-010-0048-7" @default.
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