Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...220..749t&link_type=abstract
Astrophysical Journal, Part 1, vol. 220, Mar. 15, 1978, p. 749-755. Research supported by the National Research Council.
Astronomy and Astrophysics
Astronomy
21
Background Radiation, Cosmic Gases, Galactic Clusters, Intergalactic Media, Microwave Frequencies, Compton Effect, Ionized Gases, Radio Sources (Astronomy), X Ray Sources
Scientific paper
Recently reported observations of the 3-K microwave background in the direction of rich clusters of galaxies should be viewed as placing stringent limits on the mass of cooler ionized gas within the clusters, rather than as a verification of thermal bremsstrahlung models for cluster X-ray sources. At the high radio frequencies employed in the observations, there is a positive contribution to the observed source-brightness distributions from free-free emission by any cooler gas. This can overwhelm the anticipated inverse Compton diminution of the background radiation, even when the total mass in cooler gas is significantly less than the mass of hot plasma required to explain the X-ray source. Future experiments of this type should be conducted only when atmospheric stability is sufficient to permit lengthy drift scans across the clusters. Extreme care must be taken to remove the contributions from any discrete sources.
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