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Titlebook: Astrophysics of the Diffuse Universe; Michael A. Dopita,Ralph S. Sutherland Textbook 2003 Springer-Verlag Berlin Heidelberg 2003 Astrochem

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期刊全称Astrophysics of the Diffuse Universe
影响因子2023Michael A. Dopita,Ralph S. Sutherland
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发行地址The only textbook to develop the subject matter in a pedagogical approach based on successively more complex physical systems found in the diffuse universe.Astrophysics is treated as a practical appli
学科分类Astronomy and Astrophysics Library
图书封面Titlebook: Astrophysics of the Diffuse Universe;  Michael A. Dopita,Ralph S. Sutherland Textbook 2003 Springer-Verlag Berlin Heidelberg 2003 Astrochem
影响因子Our purpose in writing this book is to show how physics has been applied to developing our current understanding of the phase structure, physical condi­ tions, chemical makeup and, evolution of the (thermal) interstellar medium. We hope it provides an up-to-date overview which postgraduates, advanced undergraduates, and professionals in astrophysics can use as a "reference of first resort" before going on to read the more specialist monographs or research literature. We have covered the exciting observational results, but without consideration of the experimental techniques or instruments required. An elementary understanding of mathematical physics and of quantum me­ chanics has been assumed, and a knowledge of basic astrophysics would be helpful. Older textbooks on interstellar physics have tended to develop the subject matter in an order which reflects the historical development of the field. Here a more pedagological approach has been adopted, based on our lecture course experience. We cover successively more complex physical systems found in the diffuse universe. Detailed mathematical rigour is eschewed in favour of provid­ ing the reader with a basic physical insight into the
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Line Transfer Effects,la. However, whether the observer can see the emission depends upon whether the nebula is optically thick or optically thin to the escape of this radiation. This in turn depends upon the ., .., of the nebula at the frequency .. For transmission of light through an absorbing screen of material, the o
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Parameters of Photoionized Regions, a wide variety of photoionized plasmas ranging from normal H. regions, planetary nebulae, and nova shells to much more exotic objects such as photoionizing shocks in metal-rich supernova remnants or active galaxies.
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