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dc.contributor.authorKelvin Lee, Kin Long
dc.contributor.authorChangala, P Bryan
dc.contributor.authorLoomis, Ryan A
dc.contributor.authorBurkhardt, Andrew M
dc.contributor.authorXue, Ci
dc.contributor.authorCordiner, Martin A
dc.contributor.authorCharnley, Steven B
dc.contributor.authorMcCarthy, Michael C
dc.contributor.authorMcGuire, Brett A
dc.date.accessioned2022-03-10T15:26:58Z
dc.date.available2022-03-10T15:26:58Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/141110
dc.description.abstract<jats:title>Abstract</jats:title> <jats:p>Using radio observations with the Green Bank Telescope, evidence has now been found for a second five-membered ring in the dense cloud Taurus Molecular Cloud-1 (TMC-1). Based on additional observations of an ongoing, large-scale, high-sensitivity spectral line survey (GOTHAM) at centimeter wavelengths toward this source, we have used a combination of spectral stacking, Markov Chain Monte Carlo (MCMC), and matched filtering techniques to detect 2-cyanocyclopentadiene, a low-lying isomer of 1-cyanocyclopentadiene, which was recently discovered there by the same methods. The new observational data also yield a considerably improved detection significance for the more stable isomer and evidence for several individual transitions between 23–32 GHz. Through our MCMC analysis, we derive cospatial, total column densities of 8.3 × 10<jats:sup>11</jats:sup> and 1.9 × 10<jats:sup>11</jats:sup> cm<jats:sup>−2</jats:sup> for 1- and 2-cyanocyclopentadiene, respectively, corresponding to a ratio of ∼4.4 favoring the former. The derived abundance ratios point toward a common formation pathway—most likely being cyanation of cyclopentadiene by analogy to benzonitrile.</jats:p>en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/2041-8213/ABE764en_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.titleInterstellar Detection of 2-cyanocyclopentadiene, C 5 H 5 CN, a Second Five-membered Ring toward TMC-1en_US
dc.typeArticleen_US
dc.identifier.citationKelvin Lee, Kin Long, Changala, P Bryan, Loomis, Ryan A, Burkhardt, Andrew M, Xue, Ci et al. 2021. "Interstellar Detection of 2-cyanocyclopentadiene, C 5 H 5 CN, a Second Five-membered Ring toward TMC-1." The Astrophysical Journal Letters, 910 (1).
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.updated2022-03-10T15:22:51Z
dspace.orderedauthorsKelvin Lee, KL; Changala, PB; Loomis, RA; Burkhardt, AM; Xue, C; Cordiner, MA; Charnley, SB; McCarthy, MC; McGuire, BAen_US
dspace.date.submission2022-03-10T15:22:53Z
mit.journal.volume910en_US
mit.journal.issue1en_US
mit.licensePUBLISHER_POLICY
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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