The Impact of Star Formation and Feedback Recipes on the Stellar Mass and Interstellar Medium of High-Redshift Galaxies
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Abstract
We introduce MEGATRON, a new galaxy formation model for cosmological radiation hydrodynamics simulations of high-redshift galaxies. The model accounts for the non-equilibrium chemistry and heating/cooling processes of ≥ 80 atoms, ions, and molecules, coupled to on-the-fly radiation transfer. We apply the model in a cosmological setting to the formation of a halo at z = 6 , and run 25 realizations at pc-scale resolution, varying numerous parameters associated with our state-of-the-art star formation, stellar feedback, and chemical enrichment models. We show that the overall budget of feedback energy is the key parameter that controls star formation regulation at high redshift, with other numerical…
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5Topics & keywords
Topics
Keywords
- Interstellar medium
- Physics
- Galaxy
- Redshift
- Astrophysics
- Star formation
- Astronomy
- Star (game theory)
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Funding
- UOUniversity of LeicesterAward: ST/K000373/1
- DUDurham UniversityAwards: ST/R000832/1, ST/S002502/1, ST/R002371/1, ST/P002293/1
- NRNational Research FoundationAward: 2022R1A6A1A03053472
- SNSwedish National Space AgencyAward: SNSA Dnr 2023-00164
- NRNational Research Foundation of KoreaAwards: 2020R1C1C1007079, 2022R1A6A1A03053472
- KOKnut och Alice Wallenbergs StiftelseAward: 2019-04659
- VVetenskapsrådetAwards: ST/K000373/1, ST/R002363/1, ST/R001014/1, 2019-04659
- SAScience and Technology Facilities CouncilAwards: ST/P002293/1, ST/R000832, ST/R002363/1, ST/R000832/1, ST/K000373/1, ST/S002502/1, ST/R001014/1, ST/R002371/1