On the time evolution of quasar luminosity and redshift distribution

Ruth Meiseles*, Ben Zion Kozlovsky, Giora Shaviv

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

The possibility to predict the redshift distribution on the basis of certain assumptions about the time-dependence of quasar luminosity is discussed. It is found that for a certain general class of models that resembles the spinar model for quasars only specific combinations of parameters give rise to acceptable results. Further consequences are discussed.

Original languageEnglish
Pages (from-to)221-231
Number of pages11
JournalAstrophysics and Space Science
Volume29
Issue number1
DOIs
StatePublished - Jul 1974

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