Comparison of X-ray and radio structure of the Cygnus Loop.

Details Comparison of X-ray and radio structure of the Cygnus Loop. Comparison of X-ray and radio structure of the Cygnus Loop.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..261l&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 261 - 262

Astronomy and Astrophysics

Astrophysics

6

Cygnus Loop: X Rays, Cygnus Loop: Radio Structure

Scientific paper

The ROSAT All-Sky Survey (RASS) is an ideal dataset to utilize in studying extended X-ray emission, in particular the emission from large angular size supernova remnants. The authors report analysis of the RASS observations of the Cygnus Loop. The complete high resolution X-ray image of the Cygnus Loop is presented. The Cygnus Loop shows X-ray emission from a more extensive region than previously appreciated, including the southern blow-out region and a newly detected western bubble. The structure of the Cygnus Loop in X-rays is compared to the radio structure observed (Leahy and Roger, 1995) using the synthesis telescope of the Dominion Radio Astrophysical Observatory, Penticton, Canada.

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