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

Rho, J.; Borkowski, K. J.

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