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- W3100774426 abstract "We derive the luminosity functions in three bands (BVR) for the rich galaxy cluster ABCG 209 at . The data cover an area of ~78 arcmin2 in the B and R bands, while a mosaic of three pointings was obtained in the V band, covering an area of approximately 160 arcmin2. The galaxy sample is complete to (), () and (). Although the fit of a single Schechter function cannot be rejected in any band, the luminosity functions are better described by a sum of two Schechter functions for bright and faint galaxies, respectively. There is an indication for a presence of a dip in the luminosity functions in the range and . We find a marked luminosity segregation, in the sense that the number ratio of bright–to–faint galaxies decreases by a factor 4 from the center to outer regions. Our analysis supports the idea that ABCG 209 is an evolved cluster, resulting from the merger of two or more sub–clusters." @default.
- W3100774426 created "2020-11-23" @default.
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- W3100774426 date "2003-09-01" @default.
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- W3100774426 title "Optical luminosity functions of the Abell galaxy cluster ABCG 209 at z = 0.21" @default.
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- W3100774426 doi "https://doi.org/10.1051/0004-6361:20030971" @default.
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