The physical origins and dominant emission mechanisms of Lyman alpha haloes: results from the TNG50 simulation in comparison to MUSE observations

The physical origins and dominant emission mechanisms of Lyman alpha haloes: results from the TNG50 simulation in comparison to MUSE observations

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Extended Lyman alpha emission is now commonly detected around high-redshift galaxies through stacking and even on individual basis. Despite recent observational advances, the physical origin of these Lyman alpha haloes (LAHs), as well as their relationships to galaxies, quasars, circumgalactic gas,...

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Bibliographic Details
Main Authors: Byrohl, Chris (Author), Nelson, Dylan (Author), Behrens, Christoph (Author), Kostyuk, Ivan (Author), Glatzle, Martin (Author), Pillepich, Annalisa (Author), Hernquist, Lars (Author), Marinacci, Federico (Author), Vogelsberger, Mark (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2022-07-07T18:10:07Z.
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