1. A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8
- Author
-
Emonts, Bjorn H. C., Lehnert, Matthew D., Yoon, Ilsang, Mandelker, Nir, Villar-Martin, Montserrat, Miley, George K., De Breuck, Carlos, Perez-Torres, Miguel A., Hatch, Nina A., and Guillard, Pierre
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The growth of galaxies in the early Universe is driven by accretion of circum- and inter-galactic gas. Simulations predict that steady streams of cold gas penetrate the dark matter halos of galaxies, providing the raw material necessary to sustain star formation. We report a filamentary stream of gas that extends for 100 kiloparsecs and connects to the massive radio galaxy 4C 41.17. The stream is detected using sub-millimeter observations of the [CI] line of atomic carbon, a tracer of neutral atomic or molecular hydrogen gas. The galaxy contains a central gas reservoir that is fueling a vigorous starburst. Our results show that the raw material for star formation can be present in cosmic streams outside galaxies., Comment: Published in Science, Volume 379, 31 March 2023 (accepted version, 31 pages)
- Published
- 2023
- Full Text
- View/download PDF