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Predictions on finding the SiH+ and SiH in interstellar space
Authors:A. A. de Almeida  P. D. Singh
Affiliation:(1) David Dunlap Observatory, University of Toronto, Toronto, Canada;(2) Present address: the Dominion Astrophysical Observatory, Victoria, B.C.
Abstract:Observations by Dressler are used to derive integral luminosity functions for ten rich clusters. All luminosity functions are found to consist of a linear portion and a high-luminosity toe. The size of this toe does not appear to correlate with cluster BM type. A parameterMF(0), which has a dispersion of only 0.2 mag for the present data sample, is defined.
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