Discovery of the elusive thioketenylium, HCCS+, in TMC-1
arXiv:2112.11855 · doi:10.1051/0004-6361/202142815
Abstract
We report the detection in TMC-1 of the cation HCCS+ (3Sigma-), which is the protonated form of the widespread radical CCS. This is the first time that a protonated radical has been detected in a cold dark cloud. Twenty-six hyperfine components from twelve rotational transitions have been observed with the Yebes 40m and IRAM 30m radio telescopes. We confidently assign the characteristic rotational spectrum pattern to HCCS+ based on the good agreement between the astronomical and theoretical spectroscopic parameters. The column density of HCCS+ is (1.1+/-0.1)e12 cm-2, and the CCS/HCCS+ abundance ratio is 50+/-10, which is very similar to that of CS/HCS+ (35+/-8) and CCCS/HCCCS+ (65+/-20). From a state-of-the-art gas-phase chemical model, we conclude that HCCS+ is mostly formed by reactions of proton transfer from abundant cations such as HCO+, H3O+, and H3+ to the radical CCS.
Accepted for publication in A&A Letters on December 21st
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- Discovery of thiofulminic acid with the QUIJOTE line survey: A study of the isomers of HNCS and HNCO in TMC-1
- Discovery of a new molecular ion, HC7NH+, in TMC-1
- A new protonated molecule discovered in TMC-1: HCCNCH+
- Discovery of five cyano derivatives of propene with the QUIJOTE line survey
- Discovery of interstellar NC4NH+: dicyanopolyynes are indeed abundant in space
- Discovery of the cyclic C5H radical in TMC-1
- Laboratory and astronomical discovery of cyanothioketene, NCCHCS, in the cold starless core TMC-1
- Linking the dust and chemical evolution: Taurus and Perseus -- New collisional rates for HCN, HNC, and their C, N, and H isotopologues
- Doubly substituted isotopologues of HCCCN in TMC-1: Detection of D13CCCN, DC13CCN, DCC13CN, DCCC15N, H13C13CCN, H13CC13CN, HC13C13CN, HCC13C15N, and HC13CC15N
- Study of the HCCNC and HNCCC isotopologs in TMC-1
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