Clumpiness of galaxies revealed in the near-infrared with COSMOS-Web
Context. Clumps in the rest-frame UV emission of galaxies at z ≲ 3 have been observed for decades. Since the launch of the James Webb Space Telescope (JWST), a large population is detected in the rest-frame near-infrared (NIR), raising questions about their formation mechanism. Aims. We investigate...
Uloženo v:
| Hlavní autoři: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
EDP Sciences
2026-02-01
|
| Edice: | Astronomy & Astrophysics |
| Témata: | |
| On-line přístup: | https://www.aanda.org/articles/aa/full_html/2026/02/aa55981-25/aa55981-25.html |
| Tagy: |
Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!
|
