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Polarimetry --- Astronomical spectroscopy --- Astronomical spectroscopy --- Polarimetry
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"This is the story of the analysis of starlight by astronomical spectroscopy, spanning from Joseph Fraunhofer's discovery of spectral lines in the early nineteenth century through to around the year 2000. In addition to the key discoveries, it presents the culture and social history of stellar astrophysics by introducing the leading astronomers, their struggles, triumphs and disagreements. Basic concepts in spectroscopy and spectral analysis are included, so both observational and theoretical aspects are described, in a non-mathematical framework. This new edition covers the final decades of the twentieth century, with its major advances in stellar astrophysics: the discovery of extrasolar planets, new classes of stars and the observation of the ultraviolet spectra of stars from satellites. The in-depth coverage of the subject makes it essential reading for graduate students working in stellar spectroscopy, as well as a major reference for professional and amateur astronomers and historians of science"--Provided by publisher.
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Double stars. --- Astronomical spectroscopy. --- Astroseismology.
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Spectroscopy enables the precise study of astronomical objects and phenomena. Bridging the gap between physics and astronomy, this is the first integrated graduate-level textbook on atomic astrophysics. It covers the basics of atomic physics and astrophysics, including state-of-the-art research applications, methods and tools. The content is evenly balanced between the physical foundations of spectroscopy and their applications to astronomical objects and cosmology. An undergraduate knowledge of physics is assumed, and relevant basic material is summarised at the beginning of each chapter. The material is completely self-contained and features sufficient background information for self-study. Advanced users will find it handy for spectroscopic studies. A website hosted by the authors contains updates, corrections, exercises and solutions, as well as news items from physics and astronomy related to spectroscopy. The text is evenly divided into atomic physics and astrophysics. The first seven chapters form the foundational elements of atomic processes and spectroscopy. The next seven chapters deal with astrophysical applications to specific objects and physical conditions. Each chapter follows the same plan. We begin with the essentials that all readers should be able to follow easily. However, towards the end of each chapter we outline some of the more advanced or specialized areas. The subject matter is broadly divided into 'basic' material in both areas, and 'advanced' material that incorporates state-of-the-art methods and results.
Atomic spectroscopy. --- Astronomical spectroscopy. --- Spectroscopie atomique --- Spectroscopie astronomique
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Stars --- Stars --- Stars --- Astronomical spectroscopy --- Atmospheres --- Atmospheres --- Mathematical models --- Spectra
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Stars --- Astronomical spectroscopy --- Spectroscopie astronomique --- Spectra --- Congresses --- Congresses --- Congrès
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Supernovae --- Astronomical spectroscopy --- Spectroscopie astronomique --- Spectra --- Congresses --- Congresses --- Congrès
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"In astronomy, spectroscopy is the technique that often provides most insight into the physical make-up of an object. In his book, Prof. Jonathan Tennyson (University College London) sets out to connect observed spectral line features to the quantummechanical properties of atoms and molecules in the line-producing, radiating media. He covers the whole electromagnetic spectrum from [gamma]-rays to radio waves. As expert in molecular spectroscopy, Tennyson puts emphasis on molecules, and the systematics in line spectra. In his foreword, he rightly stresses the role of molecules for spectra in the infrared and mm-range which are covered by (at the time of publication) upcoming observing facilities like Herschel, JWST, and ALMA. He leaves out aspects related to the modeling of spectra and the description of the instrumentation necessary for their observation. The book emerged from a lecture course for third year students. It assumes some familiarity with quantum mechanics on the level of the hydrogen atom, but not beyond. It starts out from the hydrogen atom to develop the concepts necessary to understand the spectra of complex, multi-electron systems. It applies the developed concepts to spectra observed in various astronomical environments before continuing with molecular structure and the hierarchy of molecular line spectra. Each chapter is finished by a number of problems with worked-out solutions which is helpful for lecturers using the book in their courses, or for self-study"--
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