The angular distribution of the microwave background, and its intensity in the direction of galaxy clusters

Details The angular distribution of the microwave background, and its intensity in the direction of galaxy clusters The angular distribution of the microwave background, and its intensity in the direction of galaxy clusters

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..545z&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Sept.-Oct. 1980, p. 545-547.) Soviet Astronomy Letters, vol. 6, Sept.-Oct. 1980, p.

Astronomy and Astrophysics

Astronomy

1

Angular Distribution, Background Radiation, Galactic Clusters, Microwave Scattering, Relic Radiation, Intergalactic Media, Polarization Characteristics, Quadrupoles

Scientific paper

It is noted that by observing the intensity and polarization of the
microwave background in the directions of galaxy clusters and
superclusters, it may be possible to obtain information on the angular
distribution of the background. In particular, it may be possible to
establish whether the background has a quadrupole component.

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