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dc.contributor.authorBurkhardt, Andrew M
dc.contributor.authorLong Kelvin Lee, Kin
dc.contributor.authorBryan Changala, P
dc.contributor.authorShingledecker, Christopher N
dc.contributor.authorCooke, Ilsa R
dc.contributor.authorLoomis, Ryan A
dc.contributor.authorWei, Hongji
dc.contributor.authorCharnley, Steven B
dc.contributor.authorHerbst, Eric
dc.contributor.authorMcCarthy, Michael C
dc.contributor.authorMcGuire, Brett A
dc.date.accessioned2022-03-10T15:13:30Z
dc.date.available2022-03-10T15:13:30Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/141108
dc.description.abstract<jats:title>Abstract</jats:title> <jats:p>Polycyclic aromatic hydrocarbons (PAHs) have long been invoked in the study of interstellar and protostellar sources, but the unambiguous identification of any individual PAH has proven elusive until very recently. As a result, the formation mechanisms for this important class of molecules remain poorly constrained. Here we report the first interstellar detection of a pure hydrocarbon PAH, indene (C<jats:sub>9</jats:sub>H<jats:sub>8</jats:sub>), as part of the GBT Observations of TMC-1: Hunting for Aromatic Molecules (GOTHAM) survey. This detection provides a new avenue for chemical inquiry, complementing the existing detections of CN-functionalized aromatic molecules. From fitting the GOTHAM observations, indene is found to be the most abundant organic ring detected in TMC-1 to date. And from astrochemical modeling with <jats:monospace>nautilus</jats:monospace>, the observed abundance is greater than the model’s prediction by several orders of magnitude, suggesting that current formation pathways in astrochemical models are incomplete. The detection of indene in relatively high abundance implies related species such as cyanoindene, cyclopentadiene, toluene, and styrene may be detectable in dark clouds.</jats:p>en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/2041-8213/ABFD3Aen_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceThe American Astronomical Societyen_US
dc.titleDiscovery of the Pure Polycyclic Aromatic Hydrocarbon Indene (c-C9H8) with GOTHAM Observations of TMC-1en_US
dc.typeArticleen_US
dc.identifier.citationBurkhardt, Andrew M, Long Kelvin Lee, Kin, Bryan Changala, P, Shingledecker, Christopher N, Cooke, Ilsa R et al. 2021. "Discovery of the Pure Polycyclic Aromatic Hydrocarbon Indene (c-C9H8) with GOTHAM Observations of TMC-1." The Astrophysical Journal Letters, 913 (2).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Chemistry
dc.relation.journalThe Astrophysical Journal Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-03-10T14:51:34Z
dspace.orderedauthorsBurkhardt, AM; Long Kelvin Lee, K; Bryan Changala, P; Shingledecker, CN; Cooke, IR; Loomis, RA; Wei, H; Charnley, SB; Herbst, E; McCarthy, MC; McGuire, BAen_US
dspace.date.submission2022-03-10T14:51:36Z
mit.journal.volume913en_US
mit.journal.issue2en_US
mit.licensePUBLISHER_POLICY
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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