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Title:DETECTION OF CCCH+ TOWARD W49N: ELUCIDATING THE MOLECULAR COMPLEXITY OF THE DIFFUSE INTERSTELLAR GAS
Author(s):Lee, Kelvin
Contributor(s):McCarthy, Michael C; Gupta, Harshal
Subject(s):Mini-symposium: Astrochemistry and Astrobiology in the age of ALMA
Abstract:The simple hydrocarbons CCH, $\mathrm{CCCH}$, c-$\mathrm{C_{3}H}$, $\mathrm{H_{2}CCC}$, and c-$\mathrm{C_{3}H_{2}}$ are common in the interstellar gas and are thought to be important in the production of larger molecules, yet their abundances are poorly understood. Observations of the carbon chain ion $\mathrm{CCCH^{+}}$, a key intermediate in the chemistry of these species, have begun to shed some light on their abundances: (i) maps of $\mathrm{CCCH^{+}}$ in the Horsehead nebula photodissociation region (PDR) suggest that besides ion-molecule chemistry, the fragmentation of large molecules or very small interstellar grains contributes to the production of small hydrocarbons;\footnote{Guzm{\'a}n, V., Pety, J., Goicoechea, J.~R., et al. 2015, ApJL, 800, L33} and (ii) there is important but limited evidence that the $\mathrm{CCCH^{+}}$ abundance is uniform in diffuse clouds in the Galactic disk, and is remarkably similar to $\mathrm{CCCH^{+}}$ abundances inferred in PDRs.\footnote{Gerin, M., Liszt, H., Neufeld, D., et al. 2019, A\&A, 622, A26; {\em and references therein.}} Furthermore, there is clear evidence for a very large molecule---the fullerene ion $\mathrm{C_{60}^+}$---in the diffuse gas,\footnote{Maier, J.~P. \& Campbell, E.~K. 2016, Phil. Trans. R. Soc. A, 374, (issue 2076), 1} so studies of $\mathrm{CCCH^{+}}$ and similar ions in diffuse clouds should allow robust constraints on chemistry over a very large scale in molecular size. Using the 100-m Green Bank Telescope, we recently detected the two lowest rotational transitions of $\mathrm{CCCH^{+}}$ along with transitions of several related hydrocarbons in absorption from diffuse clouds toward the luminous H~II region W49N. Our observations demonstrate that absorption spectroscopy is a highly sensitive means to detect trace polyatomic species such as $\mathrm{CCCH^{+}}$, owing to the large pathlengths through the Spiral Arms and the availability of bright centimeter continuum sources. We will discuss our results toward W49N within the context of elucidating the abundances of small hydrocarbons in diffuse clouds. We will also discuss the prospects of detecting $\mathrm{CCCH^{+}}$ toward several other Galactic continuum regions, and detecting larger polyatomic molecules in diffuse clouds through dedicated spectral line surveys.
Issue Date:2019-06-19
Publisher:International Symposium on Molecular Spectroscopy
Genre:Conference Paper / Presentation
Type:Text
Language:English
URI:http://hdl.handle.net/2142/104259
DOI:10.15278/isms.2019.WG02
Rights Information:Copyright 2019 Kelvin Lee
Date Available in IDEALS:2019-07-15
2020-01-25


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