A Detailed Comparison of X-ray and Radio Structure of the Cygnus Loop

Details A Detailed Comparison of X-ray and Radio Structure of the Cygnus Loop A Detailed Comparison of X-ray and Radio Structure of the Cygnus Loop

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....3..519l&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

The Cygnus Loop is one of the largest and nearest supernova remnants. It has been mapped by the PSPC detector of the Rontgen-Satellit ROSAT (Aschenbach and Leahy, 1999) resulting in the highest-sensitivity complete x-ray image of this remnant. The radio structure of the Cygnus Loop was observed at 1420 MHz with the synthesis telescope of the Dominion Radio Astrophysical Observatory (Leahy, Roger and Ballantyne, 1997) with similar spatial resolution. Here, is reported on a detailed comparison of the structure of the Cygnus Loop in x rays and radio.

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