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Discovery of HC 3 O + in space: The chemistry of O-bearing species in TMC-1.

Using the Yebes 40m and IRAM 30m radio telescopes, we detected a series of harmonically related lines with a rotational constant B 0 =4460.590±0.001 MHz and a distortion constant D 0 =0.511 ±0.005 kHz towards the cold dense core TMC-1. High-level-of-theory ab initio calculations indicate that the best possible candidate is protonated tricarbon monoxide, HC3 O+ . We have succeeded in producing this species in the laboratory and observed its J u - J l = 2-1 and 3-2 rotational transitions. Hence, we report the discovery of HC3 O+ in space based on our observations, theoretical calculations, and laboratory experiments. We derive an abundance ratio N (C3 O)/ N (HC3 O+ )~7. The high abundance of the protonated form of C3 O is due to the high proton affinity of the neutral species. The chemistry of O-bearing species is modelled, and predictions are compared to the derived abundances from our data for the most prominent O-bearing species in TMC-1.

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