What COBE might see - The far-infrared cosmological background

Details What COBE might see - The far-infrared cosmological background What COBE might see - The far-infrared cosmological background

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...370l...1b&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 370, March 20, 1991, p. L1-L4.

Astronomy and Astrophysics

Astronomy

38

Cosmic Background Explorer Satellite, Far Infrared Radiation, Galactic Evolution, Infrared Sources (Astronomy), Relic Radiation, Astronomical Models, Brightness Distribution, Diffuse Radiation, Emission Spectra, Red Shift

Scientific paper

The redshifted emission from infrared luminous galaxies should produce a
diffuse background around 300 microns detectable by the Cosmic
Background Explorer (COBE). The detection of such emission would provide
evidence for evolution in the density or luminosity of galaxies in the
infrared.

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