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E-grāmata: Dust and Chemistry in Astronomy

Edited by (UMIST, Manchester, UK), Edited by (UMIST, Manchester, UK)
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When astronomers got fed up trying to look at stars through the galactic dust, they started looking at the dust instead, and discovered that it plays an important role in astrochemistry. Aimed at graduate students, but potentially useful from the senior undergraduate to the practicing professional levels, 14 review articles based on lectures at a meeting in Manchester, England, January 1992, and integrating comments on them discuss aspects of dust beyond the solar system. The topics include molecular ice, carbonaceous grains, physical and chemical processes, clump collapse and star formation, and laboratory studies. Annotation copyright Book News, Inc. Portland, Or.

Dust is widespread in the galaxy. To astronomers studying stars it may be just an irritating fog, but it is becoming widely recognized that cosmic dust plays an active role in astrochemistry. Without dust, the galaxy would have evolved differently, and planetary systems like ours would not have occurred.

To explore and consolidate this active area of research, Dust and Chemistry in Astronomy covers the role of dust in the formation of molecules in the interstellar medium, with the exception of dust in the solar system. Each chapter provides thorough coverage of our understanding of interstellar dust, particularly its interaction with interstellar gas. Aimed at postgraduate researchers, the book also serves as a thorough review of this significant area of astrophysics for practicing astronomers and graduate students.

Recenzijas

"I recommend this book to those who want to catch up with the latest findings about chemical reactions occurring under conditions difficult or impossible to simulate here on Earth." -John Mathis, Science, Vol. 264, 20 May 1994

"I recommend the volume to graduate students and people entering the field." -Il Nuovo Cimento

Dust and Astrochemistry: an Introduction. Observations of Molecular Ices. Observations of Hot Molecular Cores. Molecular Hydrogen Emission from Star-Forming Regions. Carbonaceous Grains. PAHs and Astrochemistry. Physical and Chemical Processes on Dust. Interstellar Dust and the Chemistry of Diffuse Clouds. Gas-Grain Chemistry in Quiescent Dense Interstellar Clouds. The Chemistry in Low Mass Star Formation. Clump Collapse and Star Formation. The Chemistry of Hot Molecular Cores. Laboratory Dust Studies and Gas-Grain Chemistry. Irradiation of Molecular Ices.
T J Millar Department of Mathematics, UMIST, PO Box 88, Manchester M60 1QD, UK. D A Williams Department of Mathematics, UMIST, PO Box 88, Manchester M60 1QD, UK.