The energy density of the cosmic infrared background

Details The energy density of the cosmic infrared background The energy density of the cosmic infrared background

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...194...99r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 194, no. 1-2, April 1988, p. 99-101.

Astronomy and Astrophysics

Astrophysics

Galactic Clusters, Heao 1, Infrared Spectra, Polarization Characteristics, Radio Emission, X Ray Spectra, Compton Effect, Energy Transfer, Lorentz Force, Relativistic Electron Beams

Scientific paper

Improved bounds on the energy density of the infrared background are obtained by using the results of observations of diffuse intracluster radio emission, radio polarization measurements, and the results of a recent analysis of HEAO-1 hard X-ray measurements of the cluster of galaxies A 2319. If represented as a Planckian radiation field, the energy density cannot exceed 0.05, 0.15 and 0.35 eV cm-3 at 1, 10, 100 μm, respectively.

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