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DOI | 10.1126/science.1192035 |
Detection of C60and C70 in a young planetary nebula | |
Cami J.; Bernard-Salas J.; Peeters E.; Malek S.E. | |
发表日期 | 2010 |
ISSN | 0036-8075 |
起始页码 | 1180 |
结束页码 | 1182 |
卷号 | 329期号:5996 |
英文摘要 | In recent decades, a number of molecules and diverse dust features have been identified by astronomical observations in various environments. Most of the dust that determines the physical and chemical characteristics of the interstellar medium is formed in the outflows of asymptotic giant branch stars and is further processed when these objects become planetary nebulae. We studied the environment of Tc 1, a peculiar planetary nebula whose infrared spectrum shows emission from cold and neutral C60 and C70. The two molecules amount to a few percent of the available cosmic carbon in this region. This finding indicates that if the conditions are right, fullerenes can and do form efficiently in space. |
英文关键词 | carbon; carbon60; carbon70; fullerene derivative; unclassified drug; fullerene C60; fullerene C70; astronomy; carbon emission; cosmic ray; dust; outflow; physicochemical property; planetary atmosphere; article; astronomy; chemical analysis; infrared spectroscopy; physical chemistry; priority journal; temperature measurement; thermal analysis; astronomy; chemistry; microclimate; Cosmic Dust; Extraterrestrial Environment; Fullerenes; Stars, Celestial |
语种 | 英语 |
来源期刊 | Science
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/243219 |
作者单位 | Department of Physics and Astronomy, University of Western Ontario, London, ON N6A 3K7, Canada; SETI Institute, 515 North Whisman Road, Mountain View, CA 94043, United States; 222 Space Sciences Building, Cornell University, Ithaca, NY 14853, United States; Institut d'Astrophysique Spatiale, CNRS/Université Paris-Sud 11, 91405 Orsay, France |
推荐引用方式 GB/T 7714 | Cami J.,Bernard-Salas J.,Peeters E.,et al. Detection of C60and C70 in a young planetary nebula[J],2010,329(5996). |
APA | Cami J.,Bernard-Salas J.,Peeters E.,&Malek S.E..(2010).Detection of C60and C70 in a young planetary nebula.Science,329(5996). |
MLA | Cami J.,et al."Detection of C60and C70 in a young planetary nebula".Science 329.5996(2010). |
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