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Titlebook: Solid State Astrochemistry; Valerio Pirronello,Jacek Krelowski,Giulio Manicò Conference proceedings 2003 Springer Science+Business Media D

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发表于 2025-3-21 16:46:03 | 显示全部楼层 |阅读模式
书目名称Solid State Astrochemistry
编辑Valerio Pirronello,Jacek Krelowski,Giulio Manicò
视频video
丛书名称NATO Science Series II: Mathematics, Physics and Chemistry
图书封面Titlebook: Solid State Astrochemistry;  Valerio Pirronello,Jacek Krelowski,Giulio Manicò Conference proceedings 2003 Springer Science+Business Media D
描述The fundamental role that Astrochemistry plays into regulating the processes that in interstellar clouds lead to the formation of stars, and how these processes concur into affecting the shape and the dynamics of galaxies and hence into showing the Universe in the way it appears to us is well established. Together with those occurring in the gas phase a special relevance is recognized to processes that involve interstellar dust grains, the solid component of matter diffused among stars. The school on "Solid State Astrochemistry", held at the Ettore Majorana Centre for Scientific Culture in Erice (Sicily) from the 5th to the 15th of June 2000, was the fifth course of the International School of Space Chemistry. In spite of its very focused aim it was attended by 66 participants from 17 different countries, that in the very special environment provided by the Majorana Centre, discussed in great details the various aspects of the subject.
出版日期Conference proceedings 2003
关键词aromatic; aromatic hydrocarbons; astrobiology; chemistry; evolution; hydrocarbons; phase; photon; planet; pol
版次1
doihttps://doi.org/10.1007/978-94-010-0062-8
isbn_softcover978-1-4020-1559-5
isbn_ebook978-94-010-0062-8Series ISSN 1568-2609
issn_series 1568-2609
copyrightSpringer Science+Business Media Dordrecht 2003
The information of publication is updating

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https://doi.org/10.1007/978-94-010-0062-8aromatic; aromatic hydrocarbons; astrobiology; chemistry; evolution; hydrocarbons; phase; photon; planet; pol
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Trans-Neptunian Objects,The presence, the physical and dynamical properties, the chemical composition and the possible origin of Trans Neptunians small bodies are reviewd. The enrichment of dust by collisions among TNOs in the Kuiper Belt is also discussed.
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The Chemical Evolution of TMC-1,The chemical evolution in the core of contracting LS. cloud is studied to understand the observed structure in TMC-1. The results fit mostly with the observations. The possible role of gas-grain chemistry is touched.
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