Other
Scientific paper
Oct 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177..191j&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 177, Oct. 1976, p. 191-213.
Other
19
Anisotropy, Galactic Clusters, Radio Galaxies, Red Shift, Seyfert Galaxies, Spatial Distribution, Anomalies, Cosmology, Luminous Intensity, Statistical Analysis
Scientific paper
An attempt is performed to see whether the anisotropic angular distribution of redshifts discovered by Rubin, Ford, and Rubin (1973) for Sc I galaxies (denoted the RFR effect) exists for other types of sources. The data used consists of brightest cluster galaxies, those for which supernovae serve as distance indicators, and Seyfert galaxies. The statistical analysis reveals in all three cases a similar anisotropy at intermediate distances as that previously found. A modification of the RFR borderline, analyzed in particular with a complete sample of radio galaxies, shows that this anisotropy can be interpreted either as an enhancement of the luminosity, or as an excess of redshift, when galaxies are seen through intervening clusters of galaxies. This effect is evidently connected with anomalous redshifts recently discussed in the literature.
Jaakkola Toivo
Karoji Hiroshi
Le Denmat Gerard
Moles Mariano
Nottale Laurent
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