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Narrow Band Chandra X-ray Analysis of Supernova Remnant 3C391

Yang Su·Yang Chen
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Abstract

We present the narrow-band and the equivalent width (EW) images of the thermal composite supernova remnant (SNR) 3C391 for the X-ray emission lines of elements Mg, Si, & S using the Chandra ACIS Observational data. These EW images reveal the spatial distribution of the emission of the metal species Mg, Si, & S in the remnant. They have clumpy structure similar to that seen from the broadband diffuse emission, suggesting that they are largely of interstellar origin. We find an interesting finger-like feature protruding outside the southwestern radio border of the remnant, which is somewhat similar to the jet-like Si structure found in the famous SNR Cas A. This feature may possibly be the debris of the jet of ejecta which implies an asymmetrical supernova explosion of a massive progenitor star.

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Yang Su, Yang Chen. 2005-05-02. Narrow Band Chandra X-ray Analysis of Supernova Remnant 3C391. https://doi.org/10.1088/1009-9271%2F5%2F4%2F008

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