Statistical equilibrium and photospheric abundance of silicon in the Sun and in Vega

Abstract

Based on detailed non-LTE calculations, an updated determination of the abundance of silicon in the Sun and Vega is presented. The model atom includes neutral and singly ionized stages of silicon with 115 energy levels and 84 line transitions. Non-LTE eects are found to be quite small in the Sun. The mean non-LTE abundance correction is 0:010 dex with respect to standard LTE calculations, leading to a solar abundance of logNLTE =7 :550 0:056. For the prototype A0 V star Vega the non-LTE eects are small, too. With a non-LTE abundance correction of log = 0:054, a silicon abundance of logNLTE =6 :951 0:100 is derived, implying a deciency of 0:599 dex with respect to the Sun. This conrms the classication of Vega as a mild Boo star.