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A Study of the Hubble Flow

Published online by Cambridge University Press:  19 July 2016

E. Joseph Wampler
E. Joseph Wampler*
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-8046 Garching bei München, F.R.G.

Abstract

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It is found that the Hubble diagrams for quasars and giant radio galaxies are very similar. Either the evolution of giant branch stars in the galaxies closely matches the evolution of the quasar nonthermal emission or the cosmological deceleration parameter qo is close to 3.

Type
Chapter III. The Classical Quantities of Cosmology
Information
Symposium - International Astronomical Union , Volume 124: Observational Cosmology , 1987 , pp. 147 - 150
Copyright
Copyright © Reidel 1987 

References

Baldwin, J.A. 1977, Astrophys. J., 214, 679.CrossRefGoogle Scholar
Lilly, S.J., and Longair, M.S. 1984, Mon. Not. R. astr. Soc., 211, 833.CrossRefGoogle Scholar
Osmer, P., and Smith, M.G. 1980, Astrophys. J. Suppl., 42, 333.CrossRefGoogle Scholar
Schmidt, M., and Green, R.F. 1983, Astrophys. J., 269, 352.CrossRefGoogle Scholar
Wampler, E.J., Gaskell, C.M., Burke, W.L., and Baldwin, J.A. 1984, Astrophys. J., 276, 403.CrossRefGoogle Scholar
Wampler, E.J., and Ponz, D. 1985, Astrophys. J., 298, 448.CrossRefGoogle Scholar
Wampler, E.J. 1987, Astron. Astrophys., submitted.Google Scholar