Large-scale streaming motions and microwave background anisotropies

Details Large-scale streaming motions and microwave background anisotropies Large-scale streaming motions and microwave background anisotropies

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...347...11m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 347, Dec. 1, 1989, p. 11-15. Research supported by CICYT and Universidad de

Statistics

Computation

13

Computational Astrophysics, Cosmology, Radiation Distribution, Relic Radiation, Angular Distribution, Galactic Evolution, Gravitational Effects, Local Group (Astronomy), Microwave Spectra

Scientific paper

The minimal microwave background radiation is calculated on each angular scale implied by the existence of large-scale streaming motions. These minimal anisotropies, due to the Sachs-Wolfe effect, are obtained for different experiments, and give quite different results from those found in previous work. They are not in conflict with present theories of galaxy formation. Upper limits are imposed on the scale at which large-scale streaming motions can occur by extrapolating results from present double-beam-switching experiments.

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