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塵粒子上の星間ホルムアルデヒドとメタノールの形成に対する氷組成の影響
- Source :
- 第37回月・惑星シンポジウム = Proceedings of the 37th ISAS Lunar and Planetary Symposium. :91-94
- Publication Year :
- 2004
- Publisher :
- 宇宙航空研究開発機構宇宙科学研究本部, 2004.
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Abstract
- The hydrogenation of CO on pure solid CO and CO-H2O mixed ice at temperatures between 8 and 15 K is investigated by use of cold atomic hydrogen beam (30 K). The formation of H2CO and CH3OH proceeds efficiently through the hydrogenation of CO on both pure solid CO and CO-H2O mixed ice below 12 K. Around at 15 K, the hydrogenation of CO on pure solid CO is significantly suppressed, however that in CO-H2O mixed ice proceeds efficiently. Hydrogenation of CO on pure solid CO at 12 K is enhanced by a presence of H2CO molecules on the surface. H2O molecules promote a hydrogenation of CO above 12 K (up to 20 K).<br />資料番号: AA0047898024
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- 第37回月・惑星シンポジウム = Proceedings of the 37th ISAS Lunar and Planetary Symposium
- Accession number :
- edsair.jairo.........bd345d70c203ed5c03a0b92531b0d31d