Abstract

Aims.We study the oxygen and nitrogen abundances in the interstellar medium of high-redshift galaxies.Methods.We use high resolution and high signal-to-noise ratio spectra of damped Lyman-α (DLA) systems detected along the line-of-sight to quasars to derive robust abundance measurements from unsaturated metal absorption lines.Results.We present results for a sample of 16 high-redshift DLAs and strong sub-DLAs (log (H I) > 19.5, 2.4 < < 3.6) including 13 new measurements. We find that the oxygen to iron abundance ratio is pretty much constant with [O/Fe] ~ +0.320.10 for -2.5 < [O/H] < -1.0 with a small scatter around this value. The oxygen abundance follows quite well the silicon abundance within ~0.2 dex, although the silicon abundance could be slightly smaller for [O/H] . The distribution of the [N/O] abundance ratio, measured from components that are detected in both species, is somehow double peaked: five systems have [N/O] $] -1 and nine systems have [N/O] -1.15. In the diagram [N/O] versus [O/H], a loose plateau is possibly present at [N/O] ~ -0.9, which is below the so-called primary plateau as seen in local metal-poor dwarf galaxies ([N/O] in the range -0.57 to -0.74). No system is seen above this primary plateau whereas the majority of the systems lie well below with a large scatter. All this suggests a picture in which DLAs undergo successive star-bursts. During such an episode, the [N/O] ratio decreases sharply because of the rapid release of oxygen by massive stars, whereas inbetween two bursts, nitrogen is released by low and intermediate-mass stars with a delay and the [N/O] ratio increases. © 2008 ESO.