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- W4235440282 abstract "Arguments are given to support the hypothesis that a characteristic point on a cluster luminosity function, m * , corresponds to the same absolute magnitude in all clusters, and thus is an appropriate standard candle for determination of relative cluster distances. It is shown, however, that if m * is a good standard candle, then the first and tenth brightest cluster galaxies, m (1) and m (10), respectively, are not, for m * – m (1) and m * – m (10) both differ significantly from cluster to cluster. Moreover, m (1) and especially m (10) depend on cluster richness. Distances derived from them for remote clusters chosen for analysis are thus subject to selection effects that depend on cluster richness and on Bautz-Morgan type. Finally, a procedure suggested by Bautz and Abell is described whereby m * can be estimated from observed properties of distant clusters." @default.
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- W4235440282 date "1974-01-01" @default.
- W4235440282 modified "2023-09-26" @default.
- W4235440282 title "The Extragalactic Relative Distance Scale" @default.
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- W4235440282 doi "https://doi.org/10.1017/s0074180900024475" @default.
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