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ROSAT/ASCA observations of the mixed-morphology supernova remnant W28

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dc.contributor.author Rho, J. en_US
dc.contributor.author Borkowski, K. J. en_US
dc.date.accessioned 2004-09-17T05:14:49Z
dc.date.available 2004-09-17T05:14:49Z
dc.date.issued 2002
dc.identifier.citation The Astrophysical Journal en_US
dc.identifier.clearanceno 02-1112
dc.identifier.uri http://hdl.handle.net/2014/8576
dc.description.abstract 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. en_US
dc.format.extent 4581545 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other supernova remnants en_US
dc.title ROSAT/ASCA observations of the mixed-morphology supernova remnant W28 en_US


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