Interpreting Astronomical Spectra D. Emerson Institute for Astronomy, Department of Physics and Astronomy, The University of Edingurgh "Interpreting Astronomical Spectra" describes how physical conditions such as temperature, density and composition can be obtained from the spectra of a broad range of astronomical environments ranging from the cold interstellar medium to very hot coronal gas and from stellar atmospheres to quasars. In this book the author has succeeded in providing a coherent and integrated approach to the interpretation of astronomical spectroscopy, placing the emphasis on the physical understanding of spectrum formation rather than on instrumental considerations. MKS units and consistent symbols are employed throughout so that the fundamental ideas common to diverse environments are made clear and the importance of different temperature ranges and densities can be seen. Aimed at senior undergraduates and graduates studying physics, astronomy and astrophysics, this book will also appeal to the professional astronomer.
Sprache
Verlagsort
Verlagsgruppe
Zielgruppe
Für höhere Schule und Studium
Für Beruf und Forschung
Illustrationen
Maße
Höhe: 235 mm
Breite: 155 mm
Gewicht
ISBN-13
978-0-471-94176-7 (9780471941767)
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Schweitzer Klassifikation
D. Emerson Institute for Astronomy, Department of Physics and Astronomy, The University of Edinburgh
Radiative Transfer and Model Atmospheres. Microscopic Processes and Statistical Equilibrium. Line Profiles. Line Formation. Stellar Spectra. Photoionized Clouds--Gaseous Nebulae and AGN. Photoionized Clouds--AGN. The Spectrum of the Cold Interstellar Medium. Masers. Wind and Circumstellar Shells. Very Hot Thin Gases and Coronae. Appendices. Select Bibliography. Index.