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dc.contributor.authorWu, Yu-Jongen_US
dc.contributor.authorChen, Hui-Fenen_US
dc.contributor.authorCamacho, Cristopheren_US
dc.contributor.authorWitek, Henryk A.en_US
dc.contributor.authorHsu, Sheng-Chuanen_US
dc.contributor.authorLin, Meng-Yehen_US
dc.contributor.authorChou, Sheng-Lungen_US
dc.contributor.authorOgilvie, J. F.en_US
dc.contributor.authorCheng, Bing-Mingen_US
dc.date.accessioned2019-04-03T06:42:15Z-
dc.date.available2019-04-03T06:42:15Z-
dc.date.issued2009-08-10en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://dx.doi.org/10.1088/0004-637X/701/1/8en_US
dc.identifier.urihttp://hdl.handle.net/11536/149810-
dc.description.abstractPhotolysis of methane dispersed (1/1000) in solid Ne at 3 K with vacuum-ultraviolet light from a synchrotron produced infrared absorption lines of several products, including new lines at 3319.3 and 1955.5 cm(-1). Based on experiments with isotopic labeling and results of quantum-chemical calculations, these lines are assigned to the C-H stretching and C=C stretching modes, respectively, of interstellar molecule linear C5H radicals.en_US
dc.language.isoen_USen_US
dc.subjectastronomical data bases: miscellaneousen_US
dc.subjectISM: moleculesen_US
dc.subjectmolecular dataen_US
dc.subjectstars: carbonen_US
dc.titleFORMATION AND IDENTIFICATION OF INTERSTELLAR MOLECULE LINEAR C5H FROM PHOTOLYSIS OF METHANE DISPERSED IN SOLID NEONen_US
dc.typeArticleen_US
dc.identifier.doi10.1088/0004-637X/701/1/8en_US
dc.identifier.journalASTROPHYSICAL JOURNALen_US
dc.citation.volume701en_US
dc.citation.issue1en_US
dc.citation.spage8en_US
dc.citation.epage11en_US
dc.contributor.department應用化學系zh_TW
dc.contributor.department應用化學系分子科學碩博班zh_TW
dc.contributor.departmentDepartment of Applied Chemistryen_US
dc.contributor.departmentInstitute of Molecular scienceen_US
dc.identifier.wosnumberWOS:000268341800002en_US
dc.citation.woscount19en_US
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