Evolution of the barium abundance in the early Galaxy from a NLTE analysis of the Ba lines in a homogeneous sample of EMP stars

Abstract

Context. Barium is a key element in constraining the evolution of the (not well understood) r-process in the first galactic stars and currently the Ba abundances in these very metal-poor stars were mostly measured under the Local Thermodynamical Equilibrium (LTE) assumption, which may lead in general to an underestimation of Ba. Aims. We present here determinations of the barium abundance taking into account the non-LTE (NLTE) effects in a sample of extremely metal-poor stars (EMP stars): 6 turno if stars and 35 giants. Metrtods. The NLTE profiles of the three unblended Ball lines (4554 Â, 5853 Â, 6496 Â) have been computed. The computations were made with, a modified version of the MULTI code, applied to an atomic model of the Ba atom with 31 levels of Bai, 101 levels of Ball, and compared to the observations. Results. The ratios of the NLTE abundances of barium, relative to Fe are slightly shifted towards the solar ratio. In the plot of [Ba/Fe] versus [Fe/H], the slope of the regression line is slightly reduced as is the scatter. In the interval -3.3