Diffuse galactic emission

Details Diffuse galactic emission Diffuse galactic emission

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978cosp.meets....k&link_type=abstract

COSPAR, Plenary Meeting, 21st, Innsbruck, Austria, May 29-June 10, 1978, Paper. 25 p.

Physics

Diffuse Radiation, Galactic Radiation, X Ray Sources, Diagrams, Electron Energy, Emission Spectra, Energy Spectra, Gas Pressure, Interstellar Matter, Solar System, Spatial Distribution, Thermal Radiation

Scientific paper

A very large portion of the observed diffuse X-ray intensity below 1 keV
is of galactic origin. Observational evidence indicates that the
radiation is truly diffuse, is from interstellar gas near 1 million K
that is overpressured relative to the nominal interstellar pressure, and
is probably from regions close to the solar system.

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