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- W1569166780 endingPage "274" @default.
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- W1569166780 abstract "Strong Lyα emission has been detected from several different types of distant galaxies, radio galaxies and their companions at z ≃ 1.8, and galaxy companions of quasars at z > 3. This line emission is a good way of detecting galaxies at very large redshifts, and a powerful probe of the physical conditions and processes in them. A subset of the Lyα radio galaxies have photometric, spectroscopic, and morphological properties unlike those of any previously known class of objects, and may be interpreted as galaxies in the process of formation. These and other observations agree very well with some modern theoretical ideas, which predict that galaxy formation is an extended process which may begin at large redshifts, but culminate at z ~ 1–2. If this is the case, we may have already detected primeval galaxies. Searches can be (re)designed to test this notion." @default.
- W1569166780 created "2016-06-24" @default.
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- W1569166780 date "1988-01-01" @default.
- W1569166780 modified "2023-09-23" @default.
- W1569166780 title "Lyman-Alpha Galaxies at Large Redshifts" @default.
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- W1569166780 doi "https://doi.org/10.1007/978-94-009-2919-7_32" @default.
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