HELLO project: high-z evolution of large and luminous objects
We present the High-z Evolution of Large and Luminous Objects (HELLO) project, a set of $\sim \!30$ high-resolution cosmological simulations aimed to study Milky Way analogues ($M_\star \sim 10^{10-11}$ ${\mathrm{M}}_{\odot }$) at high redshift ($z\sim [2-4]$). Based on the numerical investigation o...
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| Hauptverfasser: | , , , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
September 2024
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2024, Jahrgang: 533, Heft: 2, Pages: 1463-1484 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stae1913 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: https://doi.org/10.1093/mnras/stae1913
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| Verfasserangaben: | Stefan Waterval, Andrea V. Macciò, Tobias Buck, Aura Obreja, Changhyun Cho, Zehao Jin, Benjamin L. Davis, Keri L. Dixon and Xi Kang |
| Zusammenfassung: | We present the High-z Evolution of Large and Luminous Objects (HELLO) project, a set of $\sim \!30$ high-resolution cosmological simulations aimed to study Milky Way analogues ($M_\star \sim 10^{10-11}$ ${\mathrm{M}}_{\odot }$) at high redshift ($z\sim [2-4]$). Based on the numerical investigation of a hundred astrophysical objects, HELLO features an updated scheme for chemical enrichment and the addition of local photoionization feedback. Independently of redshift and mass, our galaxies exhibit a smooth progression along the star formation main sequence until $M_\star \sim \!10^{10.5}$, around which our sample at |
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| Beschreibung: | Veröffentlicht: 08. August 2024 Gesehen am 15.10.2024 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stae1913 |