{ "id": "1706.09766", "version": "v1", "published": "2017-06-29T14:03:57.000Z", "updated": "2017-06-29T14:03:57.000Z", "title": "Detection of Interstellar HC$_5$O in TMC-1 with the Green Bank Telescope", "authors": [ "Brett A. McGuire", "Andrew M. Burkhardt", "Christopher N. Shingledecker", "Sergei V. Kalenskii", "Eric Herbst", "Anthony J. Remijan", "Michael C. McCarthy" ], "comment": "Accepted in The Astrophysical Journal Letters", "categories": [ "astro-ph.GA" ], "abstract": "We report the detection of the carbon-chain radical HC$_5$O for the first time in the interstellar medium toward the dark cloud TMC-1 using the 100 m Green Bank Telescope. We observe four hyperfine components of this radical in the $J = 17/2 \\rightarrow 15/2$ rotational transition that originates from the $^2\\Pi_{1/2}$ fine structure level of its ground state, and calculate an abundance of $n/n_{H_2}$ = $1.7\\times 10^{-10}$, assuming an excitation temperature of $T_{ex} = 7$~K. No indication of HC$_3$O, HC$_4$O, HC$_6$O, is found in these or archival observations of the source, while we report tentative evidence for HC$_7$O. We compare calculated upper limits, and the abundance of HC$_5$O to predictions based on (1) the abundance trend of the analogous HC$_n$N family in TMC-1 and (2) a gas-grain chemical model. We find that the gas-grain chemical model well reproduces the observed abundance of HC$_5$O, as well as the upper limits of HC$_3$O, HC$_6$O, and HC$_7$O, but HC$_4$O is over produced. The prospects for astronomical detection of both shorter and longer HC$_n$O chains are discussed.", "revisions": [ { "version": "v1", "updated": "2017-06-29T14:03:57.000Z" } ], "analyses": { "keywords": [ "green bank telescope", "interstellar hc", "gas-grain chemical model", "upper limits", "fine structure level" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }