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Stellar Populations in Galaxies

Published online by Cambridge University Press:  14 August 2015

Sidney Van den Bergh
Sidney Van den Bergh*
Affiliation:
David Dunlap Observatory, Toronto, Ontario, Canada

Abstract

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There are significant differences among old stellar systems which may partly be a function of luminosity. One such difference is the presence of nuclei in many high luminosity spiral galaxies but their absence in low luminosity irregular systems. Other differences are seen in the spectroscopic and photometric properties.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 44: External Galaxies and Quasi-Stellar Objects , 1972 , pp. 1 - 11
Copyright
Copyright © Reidel 1972 

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