The redshift-magnitude relation for galaxies

Details The redshift-magnitude relation for galaxies The redshift-magnitude relation for galaxies

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..33...11n&link_type=abstract

Astrophysics and Space Science, vol. 33, Mar. 1975, p. 11-21. Translation.

Astronomy and Astrophysics

Astrophysics

2

Astronomical Models, Cosmology, Galactic Clusters, Luminous Intensity, Red Shift, Astronomical Catalogs, Frequency Distribution, Hubble Diagram, Standard Deviation

Scientific paper

An analysis of magnitude-redshift data for clusters of galaxies conducted by Vignato and Marcucci (1971) is considered. The m-z plot is reexamined, taking into account both the effect of richness and B-M class. Attention is given to Friedmann models and to the steady state. For the particular problem considered, this steady state is identical with the conditions of the de Sitter cosmology.

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