paper

Deep K-band observations of TMC-1 with the Green Bank Telescope: Detection of HC7O, non-detection of HC11N, and a search for new organic molecules

arXiv:1710.10178 · doi:10.3847/1538-4357/aa970c

Abstract

The 100 m Robert C. Byrd Green Bank Telescope K-band (KFPA) receiver was used to perform a high-sensitivity search for rotational emission lines from complex organic molecules in the cold interstellar medium towards TMC-1 (cyanopolyyne peak), focussing on the identification of new carbon-chain-bearing species as well as molecules of possible prebiotic relevance. We report a detection of the carbon-chain oxide species HCO and derive a column density of ~cm. This species is theorized to form as a result of associative electron detachment reactions between oxygen atoms and CH, and/or reaction of CH with CO (followed by dissociative electron recombination). Upper limits are given for the related HCO, CO and CO molecules. In addition, we obtained the first detections of emission from individual C isotopologues of HCN, and derive abundance ratios HCN/HCCCCCCCN = and HCN/HCCCCCCCN = , indicative of significant C depletion in this species relative to the local interstellar elemental C/C ratio of 60-70. The observed spectral region covered two transitions of HCN, but emission from this species was not detected, and the corresponding column density upper limit is cm (at 95% confidence). This is significantly lower than the value of cm previously claimed by Bell et al. (1997) and confirms the recent non-detection of HCN in TMC-1 by Loomis et al. (2016). Upper limits were also obtained for the column densities of malononitrile and the nitrogen heterocycles quinoline, isoquinoline and pyrimidine.

Accepted for publication in ApJ

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