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- W3100276041 abstract "We investigated the color and morphology of optically selected galaxies in the region of clusters at z ∼ 1.2 near to the radio galaxy 3C 324 using archived data taken with the Hubble Space Telescope. The faint galaxies selected at the HST F702W band that contribute to the surface-density excess of the region have wide ranges of color, size, and morphology, which are not likely to be due to contamination by foreground galaxies. Namely, the rest-frame ultraviolet emission properties of the galaxies in the clusters are not very homogeneous; various amounts of star-formation activity may occur in a significant fraction of them. Although our analysis is purely statistical, we find that typical star-forming galaxies with blue colors have a relatively late-type morphology compared to the red quiescent population in the systems." @default.
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- W3100276041 date "1999-10-01" @default.
- W3100276041 modified "2023-09-23" @default.
- W3100276041 title "Color and Morphology of Galaxies in the Region of the 3C 324 Clusters atz∼ 1.2" @default.
- W3100276041 doi "https://doi.org/10.1093/pasj/51.5.719" @default.
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