Investigation of Galaxy and quasar luminosity evolution in the model of standard cosmology

Details Investigation of Galaxy and quasar luminosity evolution in the model of standard cosmology Investigation of Galaxy and quasar luminosity evolution in the model of standard cosmology

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.190....9t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 190, no. 1, April 1992, p. 9-22.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Luminosity, Milky Way Galaxy, Quasars, Astronomical Spectroscopy, Galactic Evolution, Hubble Diagram

Scientific paper

It is shown that the Hubble curve for Galaxies and quasars averaged over a large volume of data forms in the first approximation a single continuous curve in the interval of red shifts. A large deviation of the observed mean dependence from the theoretical one predicted by the standard cosmology is explained by the evolution of the Galaxy and especially quasar luminosity. The luminosity of the most distant of the observed quasars is on the average five to six stellar magnitudes higher than the luminosity of near galaxies and quasars. The obtained average Hubble curve of quasars and Galaxies is evidently the chief cause of their evolution in the universe.

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