ABSTRACT. This paper presents archival ROSAT PSPC observations of the G65.2+5.7 supernova remnant (also known as G65.3+5.7). Little material obscures this remnant, and so it was well observed, even at the softest end of ROSAT's bandpass (~0.11-0.28 keV). These soft X-ray images reveal the remnant's centrally filled morphology, which, in combination with existing radio frequency observations, places G65.2+5.7 in the thermal composite (mixed-morphology) class of supernova remnants. Not only might G65.2+5.7 be the oldest known thermal composite supernova remnant, but owing to its optically revealed cool, dense shell, this remnant supports the proposal that thermal composite supernova remnants lack X-ray-bright shells because they have evolved beyond the adiabatic phase. These observations also reveal a slightly extended point source centered on R.A. 19^h36^m46^s, decl. 30°40'07'' and extending 65 in radius in the band 67 map. The source of this emission has yet to be discovered, as there is no known pulsar at this location.

Subject headings: ISM: individual (G65.2+5.7); supernova remnants; X-rays: ISM

Print publication: Issue 1 (2004 November 1)
Received 2004 March 12, accepted for publication 2004 July 4