The redshift-magnitude relation for bright galaxies at low redshifts

Details The redshift-magnitude relation for bright galaxies at low redshifts The redshift-magnitude relation for bright galaxies at low redshifts

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..755s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, Sept. 1980, p. 755-767.

Mathematics

Logic

10

Cosmology, Galactic Evolution, Hertzsprung-Russell Diagram, Hubble Diagram, Red Shift, Elliptical Galaxies, Metric Space, Statistical Analysis, Stellar Luminosity

Scientific paper

Recent observations on Shapley-Ames and similar bright galaxies at low redshifts are compared with predictions based on the Hubble law and the redshift-distance square law. The phenomenological indications are unfavorable to the Hubble law, but favorable to the square law. Tests of the laws as statistical hypotheses, employing a method rigorously immune to the observational magnitude cut-off, but neglecting galaxy interdependence (clustering) reject the Hubble law at a significance level of approximately 0.001, and accept the square law.

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