An upper limit on the infrared and radio emission of clusters of galaxies

Details An upper limit on the infrared and radio emission of clusters of galaxies An upper limit on the infrared and radio emission of clusters of galaxies

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..441k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Sept.-Oct. 1978, p. 441-444.) Soviet Astronomy Letters, vol. 4, Sept.-Oct. 1978, p.

Astronomy and Astrophysics

Astronomy

Galactic Clusters, Galactic Radiation, Infrared Radiation, Millimeter Waves, Radiant Flux Density, Radio Emission, Cosmic Dust, Radiation Pressure, Space Commercialization, Spectral Line Width, Virgo Galactic Cluster

Scientific paper

A method is outlined for placing upper limits on the expected IR and millimeter-wavelength radio flux densities due to graphite dust grains in clusters of galaxies. The temperature of such dust is estimated to be around 10 K. Theoretical intensities and upper limits to spectral flux densities are computed for the Coma, Perseus, and Virgo clusters of galaxies. The results are compared with previous studies, and reasons for discrepancies between the present and previous results are considered.

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