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The growth of galaxies in the early Universe is driven by accretion ofcircum- and inter-galactic gas. Simulations predict that steady streams of coldgas penetrate the dark matter halos of galaxies, providing the raw materialnecessary to sustain star formation. We report a filamentary stream of gas thatextends 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 ofatomic carbon, a tracer of neutral atomic or molecular hydrogen gas. The galaxycontains a central gas reservoir that is fueling a vigorous starburst. Ourresults show that the raw material for star formation can be present in cosmicstreams outside galaxies.

A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8