Titlebook: Cosmo- and Geochemistry; Conference proceedings 1981 Springer-Verlag Berlin Heidelberg 1981 Geochemie.Kosmochemie.chemistry.geochemistry.

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书目名称Cosmo- and Geochemistry影响因子(影响力)




书目名称Cosmo- and Geochemistry影响因子(影响力)学科排名




书目名称Cosmo- and Geochemistry网络公开度




书目名称Cosmo- and Geochemistry网络公开度学科排名




书目名称Cosmo- and Geochemistry被引频次




书目名称Cosmo- and Geochemistry被引频次学科排名




书目名称Cosmo- and Geochemistry年度引用




书目名称Cosmo- and Geochemistry年度引用学科排名




书目名称Cosmo- and Geochemistry读者反馈




书目名称Cosmo- and Geochemistry读者反馈学科排名

汇总

Organic compounds in meteorites and their origins,solar nebula, by catalytic (Fischer-Tropsch) reactions of CO, H., and NH. at 360–400 K, ∼ 10. atm. The onset of these reactions was triggered by the formation of suitable catalysts (magnetite, hydrated silicates) at these temperatures. Such reactions may be a source of prebiotic carbon compounds on the inner planets, and interstellar molecules.

STENT

morale

verdict

外表读作

外表读作

https://doi.org/10.1007/3-540-10920-XGeochemie; Kosmochemie; chemistry; geochemistry; manganese; marine

引水渠

GRAZE

Organic compounds in meteorites and their origins,as well as heterocyclic rings containing N, O, and S. The remaining 5–30% includes the following compound classes, either present initially or generated by solvolysis: alkanes (mainly normal), alkenes, arenes, alicyclics, alcohols, aliphatic carboxylic acids, purines, pyrimidines, and other basic N-

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