期刊
PLANETARY AND SPACE SCIENCE
卷 73, 期 1, 页码 425-429出版社
PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.pss.2012.07.010
关键词
Astrobiology; Astrochemistry; Comets: general; Molecular processes; Method: laboratory; Techniques: spectroscopic
资金
- Italian Space Agency [I/015/07/0]
- LASSIE Initial Training Network
- European Community [238258]
Methyl formate is a complex organic molecule considered potentially relevant as precursor of biologically active molecules. It has been observed in several astrophysical environments, such as hot cores, hot corinos, and comets. The processes that drive the formation of molecules in cometary ices are poorly understood. In particular it is not yet clear if molecules are directly accreted from the pre-solar nebula to form comets or are formed after accretion. The present work analyzes the possible role of cosmic ion irradiation and radioactive decay in methyl formate formation in methanol-bearing ices. The results indicate that cosmic ion irradiation can account for about 12% of the methyl formate observed in comet Hale-Bopp, while radioactive decay can account for about 6% of this amount. The need of new data coming from earth based and space observational projects as well as from laboratory experiments is outlined. (C) 2012 Elsevier Ltd. All rights reserved.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据