Witnessing galaxy assembly in an extended z≈3 structure

Abstract

We present new observations acquired with the Multi Unit Spectroscopic Explorer instrument on the Very Large Telescope in a quasar field that hosts a high column-density damped Ly absorber (DLA) at z 3.25. We detect Ly emission from a nebula at the redshift of the DLA with line luminosity (27 1) 10 41 erg s -1 , which extends over 37 1 kpc above a surface brightness limit of 6 10 -19 erg s -1 cm -2 arcsec -2 at a projected distance of 30.5 0.5 kpc from the quasar sightline. Two clumps lie inside this nebula, both with Ly rest-frame equivalent width > 50 and with relative line-of-sight velocities aligned with two main absorption components seen in the DLA spectrum. In addition, we identify a compact galaxy at a projected distance of 19.1 0.5 kpc from the quasar sightline. The galaxy spectrum is noisy but consistent with that of a star-forming galaxy at the DLA redshift. We argue that the Ly nebula is ionized by radiation from star formation inside the two clumps, or by radiation from the compact galaxy. In either case, these data imply the presence of a structure with size 50 kpc inside which galaxies are assembling, a picture consistent with galaxy formation in groups and filaments as predicted by cosmological simulations such as the eagle simulations.