The submillimetre background expected from normal galaxies

Details The submillimetre background expected from normal galaxies The submillimetre background expected from normal galaxies

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..222..206e&link_type=abstract

In: After the first three minutes; Proceedings of the 1st Astrophysics Workshop, Univ. of Maryland, College Park, Oct. 15-17, 19

Astronomy and Astrophysics

Astronomy

1

Background Radiation, Cosmic Background Explorer Satellite, Galactic Radiation, Submillimeter Waves, Density Distribution, Evolution (Development), Far Infrared Radiation, Red Shift, Spaceborne Astronomy

Scientific paper

It is argued that COBE's measurements of the background emission from normal galaxies will place important limits on the strength and type of the cosmological evolution experienced by normal galaxies. It is shown that the mean intensity of the spectral shape and size of the background fluctuations all depend on the form and size of the cosmological evolution.

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