Non-Detection of HCN toward TMC-1: Constraining the Chemistry of Large Carbon-Chain Molecules
arXiv:1609.02570 · doi:10.1093/mnras/stw2302
Abstract
Bell et al. (1997) reported the first detection of the cyanopolyyne HCN toward the cold dark cloud TMC-1; no subsequent detections have been reported toward any source. Additional observations of cyanopolyynes and other carbon-chain molecules toward TMC-1 have shown a log-linear trend between molecule size and column density, and in an effort to further explore the underlying chemical processes driving this trend, we have analyzed GBT observations of HCN and HCN toward TMC-1. Although we find an HCN column density consistent with previous values, HCN is not detected and we derive an upper limit column density significantly below that reported in Bell et al. Using a state-of-the-art chemical model, we have investigated possible explanations of non-linearity in the column density trend. Despite updating the chemical model to better account for ion-dipole interactions, we are not able to explain the non-detection of HCN, and we interpret this as evidence of previously unknown carbon-chain chemistry. We propose that cyclization reactions may be responsible for the depleted HCN abundance, and that products of these cyclization reactions should be investigated as candidate interstellar molecules.
10 pages, 7 figures, 3 tables, accepted for publication in MNRAS
References in corpus (6)
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