“…We have already reported ab initio MO studies for several firstrow transition-metal-containing molecules such as FeNC [10], FeCN [11], CoCN [12,13], and NiCN [14,15] and have predicted the spectroscopic properties of the molecules, in particular the effects of the large-amplitude bending motion. For FeOH, our initial ab initio MO calculations, carried out at a highly correlated level of theory, were motivated by astrochemical interest.…”