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Concerning the Primordial Abundance of Helium in Quasi-Stellar Sources
Published online by Cambridge University Press: 14 August 2015
Abstract
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