Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....38..335d&link_type=abstract
Astronomy and Astrophysics, vol. 38, no. 3, Feb. 1975, p. 335-339.
Astronomy and Astrophysics
Astrophysics
5
Angular Velocity, Cosmology, Galactic Clusters, Gravitational Waves, Background Radiation, Brightness Temperature, Long Wave Radiation, Microwaves, Radiation Distribution, Red Shift, Spatial Distribution, Velocity Distribution
Scientific paper
Intense ultralow-frequency intergalactic gravitational radiation produces an additional component in the measured redshifts of extragalactic sources. It is noted that the near-field of gravitational waves generates, for sources with distances not exceeding one wavelength, an anisotropic and distance-dependent redshift component. This redshift field, which would have to be added to the normal redshift caused by the Hubble expansion, has some similarity with the observed redshift distribution for nearby galaxies, usually attributed to a differential rotation and expansion of the Local Supercluster. The data given by de Vaucouleurs indicate that radiation with wavelengths of the order 100 Megaparsecs could possibly be present. The local wave field also produces large-scale variations in the temperature of the cosmic microwave background radiation of quadrupole type; these variations are roughly of the order of the observed values reported by Conklin (1969, 1972).
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