Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-19T08:23:01.508Z Has data issue: false hasContentIssue false

Cosmological implication of the emission line redshift distribution of quasars*

Published online by Cambridge University Press:  19 July 2016

Y.Y. Zhou
Affiliation:
Centre for Astrophysics, Univ. of Science & Technology of China, Hefei, Anhui, China
Y. Gao
Affiliation:
Centre for Astrophysics, Univ. of Science & Technology of China, Hefei, Anhui, China
Z.G. Deng
Affiliation:
Dept. of Physics, Chinese Academy of Sciences, Beijing, China
H.J. Dai
Affiliation:
Dept. of Physics, Harbin Inst. of Technology, Harbin, China

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The peaks and dips in the quasar redshift distribution seem to be incompatible with the cosmological principle. This lays the cosmological redshift hypothesis under suspicion and censure, and has been considered by some investigators as a manifestation of the intrinsic nature of quasar's redshift. So it is worthwhile studying whether the redshift distribution of quasars could be explained in the framework of cosmological redshift. As we know, this distribution is affected not only by the possible physical origin of redshift but also by the selection effects in the observations (Zhou, Deng, Zhou 1983). From this we have the redshift distribution function f(z) = P(z)R(z), where P(z) is the real distribution function which depends on the evolutionary properties of quasars and the space-time structure of the Universe, and R(z) is the factor caused by the selection effect in the line identification.

Type
V. Cosmological Studies, Clustering, Isotropy etc
Copyright
Copyright © Reidel 1986 

References

Schmidt, M. and Green, R.F. 1983 Ap. J. 269 352 CrossRefGoogle Scholar
Zhou, Y.Y., Deng, Z.G. and Zhou, Z.L. 1983 Ap. S. S. 97 63 CrossRefGoogle Scholar
Zhou, Y.Y., Deng, Z.G. and Dai, H.J. 1985 Ap. S. S. 112 93 CrossRefGoogle Scholar