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MARC状态:已编 文献类型:西文图书 浏览次数:85

题名/责任者:
Elements of astrochemistry : chemical history of matter in the universe / edited by: Maria Emilova Velinova.
版本说明:
E-book edition.
出版发行项:
Burlington, ON : Arcler Press, 2021.
ISBN:
9781774077719 :
载体形态项:
655 pages : illustrations (some color) ; 24 cm
附加个人名称:
Velinova, Maria Emilova, editor.
论题主题:
Cosmochemistry.
中图法分类号:
P148
书目附注:
Includes bibliographical references and index.
内容附注:
Section 1: The Measurement of the Universe by Spectroscopy. Remote Sensing of Exoplanetary Atmospheres with Ground-Based High-Resolution Near-Infrared Spectroscopy ; Broadband Spectroscopy of Astrophysical ICE Analogues -- Section 2: From the Very Early Universe to the First Atoms ; Big Bang Nucleosynthesis in Visible and Hidden-Mirror Sectors ; Revisiting Big-Bang Nucleosynthesis Constraints on Long-Lived Decaying Particles -- Section 3: Stars and the Creation of the Higher Elements ; 5 Formation of the First Stars in the Universe ; Observational Constraints on the Origin of the Elements I. 3D NLTE formation of Mn lines in late-type Stars -- Section 4: Interstellar Chemistry. H2 Formation on Interstellar Dust Grains: The Viewpoints of Theory, Experiments, Models and Observations ; The First Steps of Interstellar Phosphorus Chemistry -- Section 5: Laboratory-Based Astrochemistry. GRain Surface Models and Data for Astrochemistry ; Experimental Study of the Penetration of Oxygen and Deuterium Atoms into Porous Water ICE -- Section 6: Chemistry of the Solar System. Constraining the Evolutionary History of the Moon and the Inner Solar System: a Case for New Returned Lunar Samples ; Silica-rich Volcanism in th eEarly Solar System Dated 4.565 Ga.
摘要附注:
This book reviews the recent studies on the origin and evolution of atomic matter in the Universe, considering early Universe, interstellar regions, and the solar system. In particular, it focuses on the study of the Universe by spectroscopic observations, it examines the chemical history of the very early universe to the formation of first atoms, it treats of the creation of the higher elements in the heart of the stars, and it reviews the interstellar chemistry from the viewpoints of theory, experiments, models and observations. Moreover, it provides some examples of laboratory-based astrochemistry, and at last, it focuses on the evolutionary history of the moon and the inner solar system, and their Silica-rich volcanism.
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