The Spatial Distribution Of C-2, C-3, And NH In Comet 2P/Encke

dc.contributor.utaustinauthorCochran, Anita L.en_US
dc.creatorDorman, Garretten_US
dc.creatorPierce, Donna M.en_US
dc.creatorCochran, Anita L.en_US
dc.date.accessioned2016-04-28T19:31:51Z
dc.date.available2016-04-28T19:31:51Z
dc.date.issued2013-12en
dc.description.abstractWe examine the spatial distribution of C-2, C-3, and NH radicals in the coma of comet Encke in order to understand their abundances and distributions in the coma. The observations were obtained from 2003 October 22-24, using the 2.7 m telescope at McDonald Observatory. Building on our original study of CN and OH, we have used our modified version of the vectorial model, which treats the coma as one large cone, in order to reproduce Encke's highly aspherical and asymmetric coma. Our results suggest that NH can be explained by the photodissociation of NH2, assuming that NH2 is produced rapidly from NH3 in the innermost coma. Our modeling of C-2 and C-3 suggests a multi-generational photodissociation process may be required for their production. Using the results of our previous study, we also obtain abundance ratios with respect to OH and CN. Overall, we find that Encke exhibits typical carbon-chain abundances, and the results are consistent with other studies of comet Encke.en_US
dc.description.departmentMcDonald Observatoryen_US
dc.description.sponsorshipNASA's Planetary Astronomy program grant NNXG04G162Gen_US
dc.description.sponsorshipOffice of the Vice President for Research and Economic Development at Mississippi State Universityen_US
dc.identifierdoi:10.15781/T2DN6M
dc.identifier.Filename2013_12_spatial.pdfen_US
dc.identifier.citationDorman, Garrett, Donna M. Pierce, and Anita L. Cochran. "The Spatial Distribution of C2, C3, and NH in Comet 2P/Encke." The Astrophysical Journal, Vol. 778, No. 2 (Dec., 2013): 140.en_US
dc.identifier.doi10.1088/0004-637x/778/2/140en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/2152/34653
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.relation.ispartofserialAstrophysical Journalen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.rights.restrictionOpenen_US
dc.subjectastrochemistryen_US
dc.subjectcomets: generalen_US
dc.subjectcomets: individual (encke)en_US
dc.subjectmolecularen_US
dc.subjectprocessesen_US
dc.subjectoutgassing asymmetryen_US
dc.subjectnucleusen_US
dc.subjectenckeen_US
dc.subjectatmospheresen_US
dc.subjecthalleyen_US
dc.subjectbandsen_US
dc.subjectastronomy & astrophysicsen_US
dc.titleThe Spatial Distribution Of C-2, C-3, And NH In Comet 2P/Enckeen_US
dc.typeArticleen_US

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