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- Th. Henning
- Th. Henning is at the Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäβchen 2-3, D-07745 Jena, Germany. F. Salama is at NASA Ames Research Center Space Science Division, Moffet Field, CA 94035–1000, USA.
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- F. Salama
- Th. Henning is at the Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäβchen 2-3, D-07745 Jena, Germany. F. Salama is at NASA Ames Research Center Space Science Division, Moffet Field, CA 94035–1000, USA.
書誌事項
- 公開日
- 1998-12-18
- DOI
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- 10.1126/science.282.5397.2204
- 公開者
- American Association for the Advancement of Science (AAAS)
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説明
<jats:p>Carbon is a major player in the evolutionary scheme of the universe because of its abundance and its ability to form complex species. It is also a key element in the evolution of prebiotic molecules. The different forms of cosmic carbon are reviewed ranging from carbon atoms and carbon-bearing molecules to complex, solid-state, carbonaceous structures. The current state of knowledge is assessed on the observational and laboratory fronts. Fundamental astrophysical implications are examined as well as the impact of these studies on the hitherto poorly understood physical and chemical properties of carbon materials in space.</jats:p>
収録刊行物
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- Science
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Science 282 (5397), 2204-2210, 1998-12-18
American Association for the Advancement of Science (AAAS)
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詳細情報 詳細情報について
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- CRID
- 1362544418344897920
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- NII論文ID
- 30020368033
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- ISSN
- 10959203
- 00368075
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