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dc.contributor.authorMcCarthy, Michael C
dc.contributor.authorLee, Kin Long Kelvin
dc.contributor.authorLoomis, Ryan A
dc.contributor.authorBurkhardt, Andrew M
dc.contributor.authorShingledecker, Christopher N
dc.contributor.authorCharnley, Steven B
dc.contributor.authorCordiner, Martin A
dc.contributor.authorHerbst, Eric
dc.contributor.authorKalenskii, Sergei
dc.contributor.authorWillis, Eric R
dc.contributor.authorXue, Ci
dc.contributor.authorRemijan, Anthony J
dc.contributor.authorMcGuire, Brett A
dc.date.accessioned2022-03-09T19:01:29Z
dc.date.available2022-03-09T19:01:29Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/141099
dc.description.abstract© 2020, The Author(s), under exclusive licence to Springer Nature Limited. Much like six-membered rings, five-membered rings are ubiquitous in organic chemistry, frequently serving as the building blocks for larger molecules, including many of biochemical importance. From a combination of laboratory rotational spectroscopy and a sensitive spectral line survey in the radio band toward the starless cloud core TMC-1, we report the astronomical detection of 1-cyano-1,3-cyclopentadiene (1-cyano-CPD, c-C5H5CN), a highly polar, cyano derivative of cyclopentadiene. The derived abundance of 1-cyano-CPD is far greater than predicted from astrochemical models that well reproduce the abundance of many carbon chains. This finding implies that either an important production mechanism or a large reservoir of aromatic material may need to be considered. The apparent absence of its closely related isomer, 2-cyano-1,3-cyclopentadiene, may arise from that isomer’s lower stability or may be indicative of a more selective pathway for formation of the 1-cyano isomer, perhaps one starting from acyclic precursors. The absence of N-heterocycles such as pyrrole and pyridine is discussed in light of the astronomical finding of 1-cyano-CPD.en_US
dc.language.isoen
dc.publisherSpringer Science and Business Media LLCen_US
dc.relation.isversionof10.1038/S41550-020-01213-Yen_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.sourcearXiven_US
dc.titleInterstellar detection of the highly polar five-membered ring cyanocyclopentadieneen_US
dc.typeArticleen_US
dc.identifier.citationMcCarthy, Michael C, Lee, Kin Long Kelvin, Loomis, Ryan A, Burkhardt, Andrew M, Shingledecker, Christopher N et al. 2021. "Interstellar detection of the highly polar five-membered ring cyanocyclopentadiene." Nature Astronomy, 5 (2).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Chemistry
dc.relation.journalNature Astronomyen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-03-09T18:40:28Z
dspace.orderedauthorsMcCarthy, MC; Lee, KLK; Loomis, RA; Burkhardt, AM; Shingledecker, CN; Charnley, SB; Cordiner, MA; Herbst, E; Kalenskii, S; Willis, ER; Xue, C; Remijan, AJ; McGuire, BAen_US
dspace.date.submission2022-03-09T18:40:34Z
mit.journal.volume5en_US
mit.journal.issue2en_US
mit.licensePUBLISHER_POLICY
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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