Soft X-ray emission from radio loops I and III compared

Details Soft X-ray emission from radio loops I and III compared Soft X-ray emission from radio loops I and III compared

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40..503p&link_type=abstract

(ESA, ESLAB Symposium on X-Ray Astronomy in the EXOSAT Era, 18th, The Hague, Netherlands, Nov. 5-9, 1984) Space Science Reviews

Astronomy and Astrophysics

Astronomy

Radio Sources (Astronomy), Supernova Remnants, X Ray Astronomy, Interstellar Gas, Radio Emission, Temperature Gradients

Scientific paper

The authors examine X-ray maps of the whole sky covering energies from 0.1 to 6 keV. They model Loop I X-ray emission as being caused by an old supernova that exploded into an already warm interstellar medium. After comparison with Loop III the authors deduce that there may be a general temperature gradient in the gas as one moves away from the plane in the northern galactic hemisphere.

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