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dc.contributor.authorPavithraa, S.en_US
dc.contributor.authorSahu, D.en_US
dc.contributor.authorSeth, G.en_US
dc.contributor.authorLo, J. -I.en_US
dc.contributor.authorSekhar, B. N. Rajaen_US
dc.contributor.authorCheng, B. -M.en_US
dc.contributor.authorDas, A.en_US
dc.contributor.authorMason, N. J.en_US
dc.contributor.authorSivaraman, B.en_US
dc.date.accessioned2018-08-21T05:54:19Z-
dc.date.available2018-08-21T05:54:19Z-
dc.date.issued2017-07-01en_US
dc.identifier.issn0004-640Xen_US
dc.identifier.urihttp://dx.doi.org/10.1007/s10509-017-3103-2en_US
dc.identifier.urihttp://hdl.handle.net/11536/145801-
dc.description.abstractAmong the most commonly existing thiol molecules, methanethiol and ethanethiol were discovered in the interstellar medium and identification of the next larger thiol molecule, propanethiol, is long awaited. By simulating icy astrochemical conditions and probing propanethiol ices under infrared spectroscopy we propose the use of SH stretching vibrations observed in the propanethiol molecular ice as a probe towards its identification in the interstellar medium. Though there are conformational changes within the ice (as observed in both VUV and IR spectra), the SH stretching vibration of propanethiol is observed to be unique among the set of thiol molecules, methanethiol and ethanethiol, which enables the detection of propanethiol ice in interstellar dust mantles using the James Webb Space Telescope.en_US
dc.language.isoen_USen_US
dc.subjectAstrochemistryen_US
dc.subjectTechniques: spectroscopicen_US
dc.subjectISM: moleculesen_US
dc.titleSH stretching vibration of propanethiol ice-a signature for its identification in the interstellar icy mantlesen_US
dc.typeArticleen_US
dc.identifier.doi10.1007/s10509-017-3103-2en_US
dc.identifier.journalASTROPHYSICS AND SPACE SCIENCEen_US
dc.citation.volume362en_US
dc.contributor.department應用化學系分子科學碩博班zh_TW
dc.contributor.departmentInstitute of Molecular scienceen_US
dc.identifier.wosnumberWOS:000405776700012en_US
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