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The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 pdf 下載 txt下載 epub 下載 mobi 下載 2024

The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics)
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David F. Gray 作者
Cambridge University Press
譯者
1992-06-04 出版日期
0 頁數
USD 50.00 價格
Paperback
叢書系列
9780521408684 圖書編碼

The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 圖書標籤: 天體物理學   

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發表於2024-11-05

The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 epub 下載 mobi 下載 pdf 下載 txt 下載 2024

The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 epub 下載 pdf 下載 mobi 下載 txt 下載 2024

The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 pdf 下載 txt下載 epub 下載 mobi 下載 2024


The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 用戶評價

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The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 著者簡介

The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 著者簡介

The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 pdf 下載 txt下載 epub 下載 mobi 在線電子書下載

The Observation and Analysis of Stellar Photospheres (Cambridge Astrophysics) 在線電子書 圖書描述

The starlight we see comes from the outer layers of a star, from the region known as the photosphere. Most of what we know about stars is learned by studying the light from the photosphere. This book describes the equipment, observational techniques and analysis used in the investigation of stellar photospheres. The opening chapters describe the basic tools, such as spectrographs and light detectors, as well as the physics of radiative transfer and the construction of models. Next the author introduces the measurement and modelling of the continuum spectrum. This is followed by the study of spectral line radiation. The final chapters explain how these techniques enable astronomers to deduce valuable information on basic properties of stars. For example, temperature, radius, surface gravity, chemical composition, rotation rate, and velocity fields can be derived from stellar spectroscopy. This textbook is written clearly and at a level suitable for advanced undergraduates, graduate students and researchers working on the properties of stars. The book is filled with real examples of stellar observations and analysis. There is valuable data and calibrations that are useful in real research, as well as extensive references to the primary literature.

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