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A Merger-driven Scenario for Clumpy Galaxy Formation in the Epoch of Reionization: Physical Properties of Clumps in the FirstLight Simulation

Recent JWST observations with superb angular resolution have revealed the existence of clumpy galaxies at high redshift through the detection of rest-frame optical emission lines. We use the FirstLight simulation to study the properties of (sub)galactic clumps that are bright in the [O III ] λ 5007...

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Bibliografische Detailangaben
Hauptverfasser: Yurina Nakazato, Daniel Ceverino, Naoki Yoshida
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2024-01-01
Schriftenreihe:The Astrophysical Journal
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Online-Zugang:https://doi.org/10.3847/1538-4357/ad7d0b
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