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Metal-poor Star-forming Clumps in Cosmic Noon Galaxies: Evidence for Gas Inflow and Chemical Dilution Using JWST NIRISS

The formation and evolution of galaxies are intricately linked to the baryon cycle, which fuels star formation while shaping chemical abundances within galaxies. Investigating the relationship between star formation and metallicity for large samples of galaxies requires expensive IFU surveys or soph...

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Furkejuvvon:
Váldodahkkit: Vicente Estrada-Carpenter, Marcin Sawicki, Roberto Abraham, Yoshihisa Asada, Maruša Bradač, Gabe Brammer, Guillaume Desprez, Kartheik G. Iyer, Nicholas S. Martis, Adam Muzzin, Gaël Noirot, Gregor Rihtaršič, Ghassan T. E. Sarrouh, Chris J. Willott, Jeremy Favaro, Vladan Markov, Rosa M. Mérida, Katherine Myers, Visal Sok
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: IOP Publishing 2025-01-01
Ráidu:The Astrophysical Journal
Fáttát:
Field galaxies
Chemical enrichment
Galaxy abundances
Liŋkkat:https://doi.org/10.3847/1538-4357/adfb64
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