完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.author | Chin, Chih-Hao | en_US |
dc.contributor.author | Chen, Sian-Cong | en_US |
dc.contributor.author | Liu, Meng-Chen | en_US |
dc.contributor.author | Huang, Tzu-Ping | en_US |
dc.contributor.author | Wu, Yu-Jong | en_US |
dc.date.accessioned | 2019-04-03T06:40:16Z | - |
dc.date.available | 2019-04-03T06:40:16Z | - |
dc.date.issued | 2016-06-01 | en_US |
dc.identifier.issn | 0067-0049 | en_US |
dc.identifier.uri | http://dx.doi.org/10.3847/0067-0049/224/2/17 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/134152 | - |
dc.description.abstract | We recorded the infrared and ultraviolet absorption spectra of CH4:N-2 matrix samples that underwent electron bombardment during deposition in the temperature range of 10-44 K. In contrast to a previous experiment on the IR spectroscopy of electron-bombarded icy samples, methyl and azide radicals became the main products upon electron bombardment during deposition; furthermore, reduced production of nitrile species was observed for deposition at 10 and 20 K. On the other hand, for deposition above 33 K, the observed bands of the radical species (such as methyl and azide) decreased, and bands of large nitriles appeared. This observation may suggest that radical species easily diffuse and recombine to form more complex molecules in solid nitrogen at higher temperatures. Further measurements of similar samples at 10-33 K in the UV region revealed the intense band of azide radicals at 272.5 nm and weak, broad, overlapping features of methyl and azide radicals in the 225-197 nm region. For deposition at 44 K, only a broad feature centered at 219.4 nm was observed, and the possible carriers of nitrile species were proposed based on the corresponding IR spectrum and theoretical predictions of excitation energy. This band is similar to the observed absorption feature of Pluto's surface recorded by the Hubble telescope in terms of both band position and bandwidth. Our findings therefore further support the suggestion that complex nitrile species may exist on the surface of Pluto. | en_US |
dc.language.iso | en_US | en_US |
dc.subject | astrochemistry | en_US |
dc.subject | Kuiper Belt objects: individual (Pluto) | en_US |
dc.subject | methods: laboratory: molecular | en_US |
dc.subject | molecular processes | en_US |
dc.title | INFRARED AND ULTRAVIOLET SPECTRA OF METHANE DILUTED IN SOLID NITROGEN AND IRRADIATED WITH ELECTRONS DURING DEPOSITION AT VARIOUS TEMPERATURES | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.3847/0067-0049/224/2/17 | en_US |
dc.identifier.journal | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | en_US |
dc.citation.volume | 224 | en_US |
dc.citation.issue | 2 | en_US |
dc.citation.spage | 0 | en_US |
dc.citation.epage | 0 | en_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.department | Department of Applied Chemistry | en_US |
dc.contributor.department | Institute of Molecular science | en_US |
dc.identifier.wosnumber | WOS:000381013200004 | en_US |
dc.citation.woscount | 5 | en_US |
顯示於類別: | 期刊論文 |