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 |
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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 |