TY  - GEN 
AU  - Fujimoto, S.
AU  - Espada Fernández, Daniel
PY  - 2025
UR  - https://hdl.handle.net/10481/111643
AB  - Early galaxies form through dark matter and gas assembly, evolving into dynamically hot, chaotic structures driven by mergers and feedback. By contrast, remarkably smooth, rotating disks are observed in massive galaxies only 1.4 billion years after...
LA  - eng
TI  - Primordial rotating disk composed of at least 15 dense star-forming clumps at cosmic dawn
DO  - 10.1038/s41550-025-02592-w
ER  -