Fluctuations of the cosmic background radiation at different wavelengths

Details Fluctuations of the cosmic background radiation at different wavelengths Fluctuations of the cosmic background radiation at different wavelengths

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235.1169p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Dec. 15, 1988, p. 1169-1175.

Astronomy and Astrophysics

Astronomy

1

Background Radiation, Relic Radiation, Submillimeter Waves, Autocorrelation, Cosmic Dust, Microwave Spectra, Radiation Distribution

Scientific paper

The authors analyse fluctuations of the cosmic background radiation for models with Comptonization of dust emission. To identify and constrain possible mechanisms of the origin of fluctuations they can use their correlations and amplitudes, if the fluctuations are detected at two different wavelengths. One of the wavelengths should lie in the submillimetre region, 400 μm < λ < 1.1 mm.

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