Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...255..401w&link_type=abstract
Astrophysical Journal, Part 1, vol. 255, Apr. 15, 1982, p. 401-407.
Astronomy and Astrophysics
Astrophysics
48
Big Bang Cosmology, Cosmic Dust, Microwaves, Relic Radiation, Stellar Radiation, Thermalization (Energy Absorption), Abundance, Astronomical Models, Background Radiation, Black Body Radiation, Opacity, Photoionization
Scientific paper
The possibility of the microwave background being produced by stars after the big bang is considered. The critical problem for this hypothesis is the source of the long-wavelength opacity for observed wavelengths greater than 10 cm. It is shown that free-free opacity cannot thermalize the background. Spherical dust grains also fail, but needle-shaped conducting grains can provide sufficient opacity to produce the observed spectrum with a metal abundance Z approximately equal to 10 to the -7th.
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