Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
A recent study from the Horizon Run 5 (HR5) cosmological simulation has predicted that galaxies with $\mathrm{log}\,{M}_{* }/{M}_{\odot }\lesssim 10$ in the cosmic morning (10 ≳ z ≳ 4) dominantly have disk-like morphology in the ΛCDM universe, which is driven by the tidal torque in the initial fluct...
| Κύριοι συγγραφείς: | , , , |
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| Μορφή: | Άρθρο |
| Γλώσσα: | English |
| Έκδοση: |
IOP Publishing
2024-01-01
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| Σειρά: | The Astrophysical Journal |
| Θέματα: | |
| Διαθέσιμο Online: | https://doi.org/10.3847/1538-4357/ad3448 |