Galaxy Zoo JWST: up to 75 per cent of discs are featureless at 3 < z < 7
| Autoři | |
|---|---|
| Rok publikování | 2025 |
| Druh | Článek v odborném periodiku |
| Časopis / Zdroj | Monthly Notices of the Royal Astronomical Society |
| Fakulta / Pracoviště MU | |
| Citace | |
| www | https://academic.oup.com/mnras/article/539/2/1359/8099940 |
| Doi | https://doi.org/10.1093/mnras/staf506 |
| Klíčová slova | galaxies: abundances; galaxies: disc; galaxies: elliptical and lenticular; cD; galaxies: evolution; galaxies: high-redshift; galaxies: structure |
| Přiložené soubory | |
| Popis | We have not yet observed the epoch at which disc galaxies emerge in the Universe. While high-z measurements of large-scale features such as bars and spiral arms trace the evolution of disc galaxies, such methods cannot directly quantify featureless discs in the early Universe. Here, we identify a substantial population of apparently featureless disc galaxies in the Cosmic Evolution Early Release Science (CEERS) survey by combining quantitative visual morphologies of {\sim} 7000 galaxies from the Galaxy Zoo JWST CEERS project with a public catalogue of expert visual and parametric morphologies. While the highest redshift featured disc we identify is at z_{\rm {phot}}=5.5?, the highest redshift featureless disc we identify is at z_{\rm {phot}}=7.4?. The distribution of Sérsic indices for these featureless systems suggests that they truly are dynamically cold: disc-dominated systems have existed since at least z\sim 7.4?. We place upper limits on the featureless disc fraction as a function of redshift, and show that up to 75 per?cent of discs are featureless at 3.0< z< 7.4?. This is a conservative limit assuming all galaxies in the sample truly lack features. With further consideration of redshift effects and observational constraints, we find the featureless disc fraction in CEERS imaging at these redshifts is more likely {\sim} 29{\!-\!}38~{{\ \rm per\ cent}}?. We hypothesize that the apparent lack of features in a third of high-redshift discs is due to a higher gas fraction in the early Universe, which allows the discs to be resistant to buckling and instabilities. |
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