Comparative study of low-temperature opacities with GARSTEC models
arXiv:2309.10490 · doi:10.3847/2515-5172/acf9a2
Abstract
We present a comparative study of the effect of low-temperature opacities on stellar models up to the Red Giant branch (RGB), computed with the GARching STellar Evolution Code. We have used two sets of low-temperature opacities; ÆSOPUS (Æ) from the University of Padova and those from the Wichita State University group (F05). In the relevant range of temperatures for this study, log \k{appa}Æ < log \k{appa}F 05. Therefore, to compare stellar evolutionary tracks, we performed a solar calibration of the αmlt, for each set of low-temperature opacities. After carrying such a calibration, we find that stellar evolutionary tracks are almost unaffected by the choice of low-temperature opacities, with largest variations of 25-30 K at the latest evolutionary stages of the RGB phase.