We present new abundance determinations for the sharp-lined HgMn star \chi{} Lupi A from archival FEROS spectra. Selected unblended lines with accurate atomic data have been synthesized to derive new abundances for \chi{} Lupi A. These spectra show evidence of the presence of blue-shifted lines of the companion \chi{} Lupi B. The synthesis of the spectrum of \chi{} Lupi B confirms that this star is cooler, probably an early A star with normal abundances.
@article{arxiv.1810.03460,
title = {Line identifications in the spectrum of $\chi$ Lupi A},
author = {R. Monier and T. Kılıçoğlu},
journal= {arXiv preprint arXiv:1810.03460},
year = {2018}
}
Comments
2 pages, 1 figure, accepted proceeding (poster) of SF2A2018