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ROSAT/ASCA observations of the mixed-morphology supernova remnant W28We 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.
Document ID
20060040186
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Rho, J.
Borkowski, K. J.
Date Acquired
August 23, 2013
Publication Date
January 1, 2002
Publication Information
Publication: The Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
supernova remnants

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