Non-detection of HC11N towards TMC-1: constraining the chemistry of large carbon-chain molecules. Issue 4 (12th September 2016)

• Record Type: Journal Article
• Authors: Loomis, Ryan A.; Shingledecker, Christopher N.; Langston, Glen; McGuire, Brett A.; Dollhopf, Niklaus M.; Burkhardt, Andrew M.; Corby, Joanna; Booth, Shawn T.; Carroll, P. Brandon; Turner, Barry; Remijan, Anthony J.
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 463:Issue 4(2016)
• Page Start: 4175
• Page End: 4183
• Publication Date: 2016-09-12
• Subjects: astrochemistry -- ISM: abundances -- ISM: clouds -- ISM: individual objects: TMC-1 -- ISM: molecules; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stw2302
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: Bell et al. reported the first detection of the cyanopolyyne HC11 N towards the cold dark cloud TMC-1; no subsequent detections have been reported towards any source. Additional observations of cyanopolyynes and other carbon-chain molecules towards 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 analysed Green Bank Telescope observations of HC9 N and HC11 N towards TMC-1. Although we find an HC9 N column density consistent with previous values, HC11 N 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 HC11 N, and we interpret this as evidence of previously unknown carbon-chain chemistry. We propose that cyclization reactions may be responsible for the depleted HC11 N abundance, and that products of these cyclization reactions should be investigated as candidate interstellar molecules.