dc.contributor.author | Kelvin Lee, Kin Long | |
dc.contributor.author | Changala, P Bryan | |
dc.contributor.author | Loomis, Ryan A | |
dc.contributor.author | Burkhardt, Andrew M | |
dc.contributor.author | Xue, Ci | |
dc.contributor.author | Cordiner, Martin A | |
dc.contributor.author | Charnley, Steven B | |
dc.contributor.author | McCarthy, Michael C | |
dc.contributor.author | McGuire, Brett A | |
dc.date.accessioned | 2022-03-10T15:26:58Z | |
dc.date.available | 2022-03-10T15:26:58Z | |
dc.date.issued | 2021 | |
dc.identifier.uri | https://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.iso | en | |
dc.publisher | American Astronomical Society | en_US |
dc.relation.isversionof | 10.3847/2041-8213/ABE764 | en_US |
dc.rights | Article 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.source | The American Astronomical Society | en_US |
dc.title | Interstellar Detection of 2-cyanocyclopentadiene, C 5 H 5 CN, a Second Five-membered Ring toward TMC-1 | en_US |
dc.type | Article | en_US |
dc.identifier.citation | Kelvin 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.department | Massachusetts Institute of Technology. Department of Chemistry | |
dc.relation.journal | The Astrophysical Journal Letters | en_US |
dc.eprint.version | Final published version | en_US |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
dc.date.updated | 2022-03-10T15:22:51Z | |
dspace.orderedauthors | Kelvin Lee, KL; Changala, PB; Loomis, RA; Burkhardt, AM; Xue, C; Cordiner, MA; Charnley, SB; McCarthy, MC; McGuire, BA | en_US |
dspace.date.submission | 2022-03-10T15:22:53Z | |
mit.journal.volume | 910 | en_US |
mit.journal.issue | 1 | en_US |
mit.license | PUBLISHER_POLICY | |
mit.metadata.status | Authority Work and Publication Information Needed | en_US |