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  • 1
    Publication Date: 2018-06-08
    Description: We present three sets of ROSAT PSPC and four sets of ASCA observations of the supernova remnant (SNR) W28. The overall shape of x-ray emission in W28 is elliptical, dominated by a centrally-concentrated interior emission, sharply peaked at the center. There are also partial northeastern and southwestern shells, and both central and shell x-ray emission is highly patchy.
    Keywords: Astrophysics
    Type: The Astrophysical Journal
    Format: text
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