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Historical Introduction
Published online by Cambridge University Press: 12 April 2016
Abstract
Our ideas about the surface brightness distribution of galaxies has changed greatly since 1970. I contrast the view at that time with our present view of the subject, and then briefly discuss some topics in the studies of Low Surface Brightness Galaxies (LSBG) that I think are particularly interesting: the Tully-Fisher relation, LSBG as systems of high angular momentum, LSBG in clusters of galaxies, and the potential impact of the HIPASS survey.
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- Observational selection effects
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- Copyright © Astronomical Society of the Pacific 1999