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DOI | 10.1126/science.1071136 |
Polytype distribution in circumstellar silicon carbide | |
Daulton T.L.; Bernatowicz T.J.; Lewis R.S.; Messenger S.; Stadermann F.J.; Amari S. | |
发表日期 | 2002 |
ISSN | 0036-8075 |
起始页码 | 1852 |
结束页码 | 1855 |
卷号 | 296期号:5574 |
英文摘要 | The inferred crystallographic class of circumstellar silicon carbide based on astronomical infrared spectra is controversial. We have directly determined the polytype distribution of circumstellar SiC from transmission electron microscopy of presolar silicon carbide from the Murchison carbonaceous meteorite. Only two polytypes (of a possible several hundred) were observed: cubic 3C and hexagonal 2H silicon carbide and their intergrowths. We conclude that this structural simplicity is a direct consequence of the low pressures in circumstellar outflows and the corresponding low silicon carbide condensation temperatures. |
英文关键词 | Astrophysics; Crystal growth; Crystallography; Meteorites; Transmission electron microscopy; Polytypes; Silicon carbide; silicon carbide; silicon; transmission electron microscopy; article; crystallography; grain; infrared spectroscopy; polymerization; priority journal; temperature; transmission electron microscopy; Astronomy; Carbon Compounds, Inorganic; Meteoroids; Microscopy, Electron; Pressure; Silicon Compounds; Temperature |
语种 | 英语 |
来源期刊 | Science |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/243464 |
作者单位 | Materials Science Division, Argonne National Laboratory, Argonne IL, 60439-4838, United States |
推荐引用方式 GB/T 7714 | Daulton T.L.,Bernatowicz T.J.,Lewis R.S.,et al. Polytype distribution in circumstellar silicon carbide[J],2002,296(5574). |
APA | Daulton T.L.,Bernatowicz T.J.,Lewis R.S.,Messenger S.,Stadermann F.J.,&Amari S..(2002).Polytype distribution in circumstellar silicon carbide.Science,296(5574). |
MLA | Daulton T.L.,et al."Polytype distribution in circumstellar silicon carbide".Science 296.5574(2002). |
条目包含的文件 | 条目无相关文件。 |
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