Distortion of the microwave background by a hot intergalactic medium

Details Distortion of the microwave background by a hot intergalactic medium Distortion of the microwave background by a hot intergalactic medium

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...232..348w&link_type=abstract

Astrophysical Journal, Part 1, vol. 232, Sept. 1, 1979, p. 348-351.

Astronomy and Astrophysics

Astronomy

85

Background Radiation, Intergalactic Media, Microwaves, X Ray Astronomy, Cosmic X Rays, Electrons, Frequency Shift, Velocity Distribution

Scientific paper

The distortion of the cosmic microwave background by a hot, optically
thin intergalactic medium (IGM) is calculated using the full frequency
redistribution function. Even if the IGM produces all of the cosmic
X-ray background, the distortion of the microwave background is not
detectable in the present observational data.

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