Introduction to Astronomical Spectroscopy
Spectroscopy is the principal tool used in astronomy to investigate the Universe beyond Earth's atmosphere. Through the analysis of electromagnetic radiation, spectrographs enable observers to assess the chemical composition, kinematics, and local physical properties of distant stars, nebulae, and galaxies. Thoroughly illustrated and clearly written, this handbook offers a practical and comprehensive guide to the different spectroscopic methods used in all branches of astronomy, at all wavelengths from radio to gamma-ray, and from ground and space-borne instruments. After a historical overview of the field, the central chapters navigate the various types of hardware used in spectroscopy. In-depth descriptions of modern techniques and their benefits and drawbacks help you choose the most promising observation strategy. The handbook finishes by assessing new technologies and future prospects for deep-sky observation. This text is an ideal reference for today's graduate students and active researchers, as well as those designing or operating spectroscopic instruments.
1118726033
Introduction to Astronomical Spectroscopy
Spectroscopy is the principal tool used in astronomy to investigate the Universe beyond Earth's atmosphere. Through the analysis of electromagnetic radiation, spectrographs enable observers to assess the chemical composition, kinematics, and local physical properties of distant stars, nebulae, and galaxies. Thoroughly illustrated and clearly written, this handbook offers a practical and comprehensive guide to the different spectroscopic methods used in all branches of astronomy, at all wavelengths from radio to gamma-ray, and from ground and space-borne instruments. After a historical overview of the field, the central chapters navigate the various types of hardware used in spectroscopy. In-depth descriptions of modern techniques and their benefits and drawbacks help you choose the most promising observation strategy. The handbook finishes by assessing new technologies and future prospects for deep-sky observation. This text is an ideal reference for today's graduate students and active researchers, as well as those designing or operating spectroscopic instruments.
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Introduction to Astronomical Spectroscopy

Introduction to Astronomical Spectroscopy

by Immo Appenzeller
Introduction to Astronomical Spectroscopy

Introduction to Astronomical Spectroscopy

by Immo Appenzeller

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Overview

Spectroscopy is the principal tool used in astronomy to investigate the Universe beyond Earth's atmosphere. Through the analysis of electromagnetic radiation, spectrographs enable observers to assess the chemical composition, kinematics, and local physical properties of distant stars, nebulae, and galaxies. Thoroughly illustrated and clearly written, this handbook offers a practical and comprehensive guide to the different spectroscopic methods used in all branches of astronomy, at all wavelengths from radio to gamma-ray, and from ground and space-borne instruments. After a historical overview of the field, the central chapters navigate the various types of hardware used in spectroscopy. In-depth descriptions of modern techniques and their benefits and drawbacks help you choose the most promising observation strategy. The handbook finishes by assessing new technologies and future prospects for deep-sky observation. This text is an ideal reference for today's graduate students and active researchers, as well as those designing or operating spectroscopic instruments.

Product Details

ISBN-13: 9781107601796
Publisher: Cambridge University Press
Publication date: 12/17/2012
Series: Cambridge Observing Handbooks for Research Astronomers , #9
Edition description: New Edition
Pages: 268
Product dimensions: 6.00(w) x 8.90(h) x 0.50(d)

About the Author

Immo Appenzeller is Emeritus Professor of Astronomy at the University of Heidelberg, Germany, and Director of the Heidelberg State Observatory.

Table of Contents

Preface; 1. Historical remarks; 2. Spectroscopy in present-day astronomy; 3. Basic physics of spectral measurements; 4. Optical-range grating and prism spectrometers; 5. Other techniques for the optical spectral range; 6. Preparing and reducing optical observations; 7. UV, X-ray, and gamma spectroscopy; 8. Spectroscopy at radio wavelengths; 9. Special techniques for the far IR and sub-mm range; 10. New developments and future prospects; Appendix; List of references; Index.
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