Possible explanations of the large angle fluctuations of the microwave background

Details Possible explanations of the large angle fluctuations of the microwave background Possible explanations of the large angle fluctuations of the microwave background

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...399l...9h&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 399, no. 1, p. L9, L10.

Astronomy and Astrophysics

Astrophysics

5

Cosmology, Microwaves, Milky Way Galaxy, Relic Radiation, Astronomical Models, Cosmic Dust, Dark Matter

Scientific paper

Possible origins of the structure in the cosmic microwave background radiation are discussed. It is pointed out that the presence of such structure is compatible with the 1990 modified steady state model proposed by Arp et al. The possibility that the fluctuations are due to dust grains in the form of iron whiskers produced comparatively locally is also discussed.

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