Limits on diffuse X-ray emission from M101

Details Limits on diffuse X-ray emission from M101 Limits on diffuse X-ray emission from M101

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...287..167m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 287, Dec. 1, 1984, p. 167-174. Previously announced in STAR as N84-18147.

Astronomy and Astrophysics

Astrophysics

39

Diffuse Radiation, Galactic Radiation, Interstellar Matter, Spiral Galaxies, X Rays, Coronas, High Temperature Gases, Interstellar Gas, Milky Way Galaxy, Supernovae

Scientific paper

Observed limits on diffuse X-ray emission from M101 require that the temperature of any coronal or matrix hot gas that is radiating an appreciable part (⪆10%) of the average supernova power be less than 105.7K. Furthermore, the fraction of the galactic plane occupied by hot bubbles similar to the one that apparently surrounds the Sun is at most 25% in the region between 10 kpc and 20 kpc from the galactic center.

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