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G65.2+5.7: A Thermal Composite Supernova Remnant with a Cool Shell

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R. L. Shelton1, K. D. Kuntz2 and R. Petre3

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[1]

Far-ultraviolet Emission-line Morphologies of the Supernova Remnant G65.3+5.7

I.-J. Kim et al.  The Astrophysical Journal 2010  722 388
IOPscience 
[2]

An X-Ray Search for Compact Central Sources in Supernova Remnants. II. Six Large-Diameter SNRs

D. L. Kaplan et al.  The Astrophysical Journal Supplement Series 2006  163 344
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[3]

Enhanced Abundances in Three Large-Diameter Mixed-Morphology Supernova Remnants

J. S. Lazendic and P. O. Slane  The Astrophysical Journal 2006  647 350
IOPscience 
[4]

Simulations of Supernova Remnants in Diffuse Media. III. The Population of Buoyant Remnants above the Milky Way's Disk

R. L. Shelton  The Astrophysical Journal 2006  638 206
IOPscience 
[5]

Ionization States and Plasma Structures of Mixed-Morphology Supernova Remnants Observed with ASCA

Masahiro Kawasaki et al.  The Astrophysical Journal 2005  631 935
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