Faint extended Lyalpha emission due to star formation at the centre of high-column density QSO absorption systems

TL;DR

This study uses radiative transfer models to confirm that faint Lyalpha emission around DLAs originates from star formation in low-mass dark matter halos, explaining their spatial extent and properties.

Contribution

It presents a detailed radiative transfer model that reproduces observed DLA and Lyalpha emitter properties, linking star formation to faint Lyalpha emission in low-mass halos.

Findings

DLAs are hosted by dark matter halos of 10^{9.5}-10^{12} solar masses.

Star formation in halos causes faint Lyalpha emission with large spatial extent.

Lyalpha emission has a duty cycle of approximately 25%.

Abstract

We use detailed Lyalpha radiative transfer calculations to further test the claim of Rauch et al. (2008) that they have detected spatially extended faint Lyalpha emission from the elusive host population of Damped Lyalpha Absorption systems (DLAs) in their recent ultra-deep spectroscopic survey. We investigate the spatial and spectral distribution of Lyalpha emission due to star-formation at the centre of DLAs, and its dependence on the spatial and velocity structure of the gas. Our model simultaneously reproduces the observed properties of DLAs and the faint Lyalpha emitters, including the velocity width and column density distribution of DLAs and the large spatial extent of the emission of the faint emitters. Our modelling confirms previous suggestions that DLAs are predominately hosted by Dark Matter (DM) halos in the mass range 10^{9.5}-10^{12} M_sun, and are thus of significantly lower mass than those inferred for L_* Lyman Break Galaxies (LBGs). Our modelling suggests that DM halos hosting DLAs retain up to 20% of the cosmic baryon fraction in the form of neutral hydrogen, and that star formation at the centre of the halos is responsible for the faint Lyalpha emission. The scattering of a significant fraction of the Lyalpha emission to the observed radii, which can be as large as 50 kpc or more, requires the amplitude of the bulk motions of the gas at the centre of the halos to be moderate. The observed space density and size distribution of the emitters together with the incidence rate of DLAs suggests that the Lyalpha emission due to star formation has a duty cycle of ~ 25%.