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dc.contributorVirginia Tech
dc.contributor.authorFortenberry, R. C.
dc.contributor.authorHuang, X. C.
dc.contributor.authorCrawford, T. Daniel
dc.contributor.authorLee, T. J.
dc.date.accessioned2014-02-25T13:57:04Z
dc.date.available2014-02-25T13:57:04Z
dc.date.issued2013-07
dc.identifier.citationRyan C. Fortenberry et al. 2013. "high-accuracy quartic force field calculations for the spectroscopic constants and vibrational frequencies of 1(1)a ' l-c3h-: a possible link to lines observed in the horsehead nebula photodissociation region," ApJ 772 39 doi:10.1088/0004-637X/772/1/39
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/10919/25549
dc.description.abstractIt has been shown that rotational lines observed in the Horsehead nebula photodissociation region (PDR) are probably not caused by l-C3H+, as was originally suggested. In the search for viable alternative candidate carriers, quartic force fields are employed here to provide highly accurate rotational constants, as well as fundamental vibrational frequencies, for another candidate carrier: 1(1)A'C3H-. The ab initio computed spectroscopic constants provided in this work are, compared to those necessary to define the observed lines, as accurate as the computed spectroscopic constants for many of the known interstellar anions. Additionally, the computed D-eff for C3H is three times closer to the D deduced from the observed Horsehead nebula lines relative to l-C3H+. As a result, 1(1)A'C3H- is a more viable candidate for these observed rotational transitions. It has been previously proposed that at least C6H- may be present in the Horsehead nebular PDR formed by way of radiative attachment through its dipole-bound excited state. C3H- could form in a similar way through its dipole-bound state, but its valence excited state increases the number of relaxation pathways possible to reach the ground electronic state. In turn, the rate of formation for C3H- could be greater than the rate of its destruction. C3H- would be the seventh confirmed interstellar anion detected within the past decade and the first CnH- molecular anion with an odd n.
dc.description.sponsorshipNASA
dc.description.sponsorshipNASA/SETI Institute NNX12AG96A
dc.description.sponsorshipNASA's Laboratory Astrophysics "Carbon in the Galaxy" Consortium Grant NNH10ZDA001N
dc.description.sponsorshipU.S. National Science Foundation (NSF) Multi-User Chemistry Research Instrumentation and Facility (CRIF:MU) award CHE-0741927, NSF-1058420
dc.language.isoen_US
dc.publisherIOP Publishing Ltd.
dc.subjectastrochemistry
dc.subjectism: individual objects (horsehead nebula)
dc.subjectism: lines
dc.subjectand bands
dc.subjectism: molecules
dc.subjectmolecular data
dc.subjectradio lines: ism
dc.subjectcorrelated molecular calculations
dc.subjectgaussian-basis sets
dc.subjectastronomical
dc.subjectdetection
dc.subjectelectron-attachment
dc.subjectinterstellar clouds
dc.subjectexcited-states
dc.subjectanions
dc.subjectc4h
dc.subjectatoms
dc.subjectenergy
dc.titlehigh-accuracy quartic force field calculations for the spectroscopic constants and vibrational frequencies of 1(1)a ' l-c3h-: a possible link to lines observed in the horsehead nebula photodissociation region
dc.typeArticle - Refereed
dc.identifier.urlhttp://m.iopscience.iop.org/0004-637X/772/1/39/pdf/0004-637X_772_1_39.pdf
dc.date.accessed2014-02-05
dc.title.serialAstrophysical Journal
dc.identifier.doihttps://doi.org/10.1088/0004-637x/772/1/39


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