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Environmental Effects on the Faint End of the Luminosity Function
Published online by Cambridge University Press: 12 April 2016
Abstract
Recent studies have demonstrated that many galaxy clusters have luminosity functions (LFs) which are steep at the faint end. However, it is equally clear that not all clusters have identical LFs. In this paper we explore whether the variation in LF shape correlates with other cluster or environmental properties.
- Type
- Properties of Low Surface Brightness galaxies
- Information
- International Astronomical Union Colloquium , Volume 171: The Low Surface Brightness Universe , 1999 , pp. 183 - 190
- Copyright
- Copyright © Astronomical Society of the Pacific 1999