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Concerning the Primordial Abundance of Helium in Quasi-Stellar Sources

Published online by Cambridge University Press:  14 August 2015

Joseph Silk
Joseph Silk*
Affiliation:
Princeton University Observatory, N.J., U.S.A.

Abstract

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Primordial temperature fluctuations, which appear to be necessary in order to explain aspects of galaxy formation, can lead to observable effects in some objects. In QSS and other compact systems a correlation of absolute luminosity with primordial helium content is predicted.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 44: External Galaxies and Quasi-Stellar Objects , 1972 , pp. 474 - 477
Copyright
Copyright © Reidel 1972 

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