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- W100516103 abstract "Possibilities for detecting primaeval galaxies are reviewed. The best prospects for detection are giant elliptical galaxies, in a stage of rapid star formation about 10 10 years ago. These primaeval galaxies would probably be quasi-stellar in angular size. They could have easily detectable magnitudes if the most luminous stage occurs at red shifts z ≤ 5, and if internal dust does not absorb most of the ultraviolet—visual light. Although it is not clear whether very young giant elliptical galaxies have yet been found, excess populations of blue galaxies in clusters (discovered by Butcher & Oemler) and in the field (discovered by Kron) are almost certainly in early stages of active star formation." @default.
- W100516103 created "2016-06-24" @default.
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- W100516103 date "1980-03-06" @default.
- W100516103 modified "2023-09-27" @default.
- W100516103 title "The detectability of young galaxies" @default.
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- W100516103 doi "https://doi.org/10.1098/rsta.1980.0173" @default.
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