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dc.contributor.authorPavithraa, S.en_US
dc.contributor.authorLo, J-Ien_US
dc.contributor.authorRahul, K.en_US
dc.contributor.authorSekhar, B. N. Rajaen_US
dc.contributor.authorCheng, B-M.en_US
dc.contributor.authorMason, N. J.en_US
dc.contributor.authorSivaraman, B.en_US
dc.date.accessioned2018-08-21T05:52:56Z-
dc.date.available2018-08-21T05:52:56Z-
dc.date.issued2018-02-05en_US
dc.identifier.issn1386-1425en_US
dc.identifier.urihttp://dx.doi.org/10.1016/j.saa.2017.08.060en_US
dc.identifier.urihttp://hdl.handle.net/11536/144108-
dc.description.abstractHere we present the first Vacuum UltraViolet (VUV) photoabsorption spectra of ice analogues of Pluto and Charon ice mixtures. For Pluto the ice analogue is an icy mixture containing nitrogen (N-2), carbon monoxide (CO), methane (CH4) and water (H2O) prepared with a 100:1:1:3 ratio, respectively. Photoabsorption of icy mixtures with and without H2O were recorded and no significant changes in the spectra due to presence of H2O were observed. For Charon a VUV photoabsorption spectra of an ice analogue containing ammonia (NH3) and H2O prepared with a 1:1 ratio was recorded, a spectrum of ammonium hydroxide (NH4OH) was also recorded. These spectra may help to interpret the P-Alice data from New Horizons. (C) 2017 Elsevier B.V. All rights reserved.en_US
dc.language.isoen_USen_US
dc.subjectAstrochemistry methodsen_US
dc.subjectLaboratoryen_US
dc.subjectSolid state techniquesen_US
dc.subjectSpectroscopicen_US
dc.titleVacuum ultraviolet photoabsorption of prime ice analogues of Pluto and Charonen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.saa.2017.08.060en_US
dc.identifier.journalSPECTROCHIMICA ACTA PART A-MOLECULAR AND BIOMOLECULAR SPECTROSCOPYen_US
dc.citation.volume190en_US
dc.citation.spage172en_US
dc.citation.epage176en_US
dc.contributor.department交大名義發表zh_TW
dc.contributor.departmentNational Chiao Tung Universityen_US
dc.identifier.wosnumberWOS:000415912500023en_US
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