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- W3033627369 abstract "Abstract Characterising primeval galaxies entails the challenging goal of observing galaxies with modest star formation rates (S FR < 100 M ȯ yr −1 ) and approaching the beginning of the reionisation epoch ( z > 6). To date a large number of primeval galaxies have been identified thanks to deep near-infrared surveys. However, to further our understanding on the formation and evolution of such primeval objects, we must investigate their nature and physical properties through multi-band spectroscopic observations. Information on dust content, metallicity, interactions with the surrounding environment, and outflows can be obtained with ALMA observations of far-infrared (FIR) lines such as the [C ii ] at 158 μ m and [O iii ] at 88 μ m. Here, we, thus, discuss the recent results unveiled by ALMA observations and present new [C ii ] observations of BDF-3299, a star-forming galaxy at z = 7.1 showing a spatial and spectral offset between the rest-frame UV and the FIR lines emission." @default.
- W3033627369 created "2020-06-12" @default.
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- W3033627369 date "2019-06-01" @default.
- W3033627369 modified "2023-10-18" @default.
- W3033627369 title "ALMA witnesses the assembly of first galaxies" @default.
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- W3033627369 doi "https://doi.org/10.1017/s1743921319009098" @default.
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