On the anisotropy of the cosmic microwave background

Details On the anisotropy of the cosmic microwave background On the anisotropy of the cosmic microwave background

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...423...19m&link_type=abstract

The Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 423, no. 1, p. 19-21

Astronomy and Astrophysics

Astrophysics

16

Anisotropy, Background Radiation, Cosmic Rays, Cosmology, Microwave Emission, Universe, Baryons, Cosmic Background Explorer Satellite, Mass Distribution, Photons, Red Shift, Symmetry

Scientific paper

It is likely that the anisotropy of the cosmic microwave background -- discovered by the Cosmic Background Explorer (COBE) satellite -- is due to near structures (voids, superclusters, etc., at redshift less than 2) and has nothing in common with the distribution of matter at redshift approximately or equal to 1000. This result follows from the analytic calculation of the redshift of light that crosses a spherical void.

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