The millimeter/submillimeter spectrum of the molecular ion FeCO + ( X 4 Σ - ) has been recorded using velocity modulation spectroscopy. The molecular ion was created in an AC discharge of Fe(CO) 5 and argon. Twenty-seven rotational transitions, each consisting of four fine-structure components, were measured in the range 198-418 GHz. The data were fit with a case b Hamiltonian, and rotational, spin-rotation, and spin-spin constants were determined. Because of the presence of higher order spin-orbit interactions, probably caused in part by a nearby 4 Π excited state, numerous centrifugal distortion terms were needed for the spectral analysis. The value of γ s , the third-order spin-rotation constant, was also remarkably large at -72.4 MHz. Rest frequencies for FeCO + are now available for interstellar and circumstellar searches. This species may be present in molecular clouds, where CO is abundant and gas-phase iron should be in the form of Fe + . Molecular ions such as FeCO + could be the hidden carriers of metallic elements in such clouds.
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Halfen et al. (2007) studied this question.
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