Stellar Motions - Campbell, William Wallace
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Stellar Motions: With Special Reference To Motions Determined By Means Of The Spectrograph (1913) is a book written by William Wallace Campbell. In this book, Campbell explores the topic of stellar motions, particularly those determined by the use of the spectrograph. The book is divided into several chapters, each of which covers a different aspect of the topic. The first chapter provides an introduction to the subject, discussing the history of the study of stellar motions and the various methods that have been used to determine them. The second chapter focuses on the spectrograph and how it…mehr

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Stellar Motions: With Special Reference To Motions Determined By Means Of The Spectrograph (1913) is a book written by William Wallace Campbell. In this book, Campbell explores the topic of stellar motions, particularly those determined by the use of the spectrograph. The book is divided into several chapters, each of which covers a different aspect of the topic. The first chapter provides an introduction to the subject, discussing the history of the study of stellar motions and the various methods that have been used to determine them. The second chapter focuses on the spectrograph and how it is used to measure stellar motions. Campbell explains the principles behind the spectrograph and provides examples of how it has been used in the past.The following chapters delve deeper into the topic of stellar motions, discussing the different types of motions that can be observed and the factors that influence them. Campbell also provides examples of how spectroscopic observations have been used to determine the motions of specific stars and star systems.Overall, Stellar Motions: With Special Reference To Motions Determined By Means Of The Spectrograph (1913) is a comprehensive guide to the study of stellar motions. It provides a detailed explanation of the spectrograph and its use in determining stellar motions, as well as a thorough exploration of the different types of motions that can be observed. This book is a valuable resource for anyone interested in the study of astronomy and astrophysics.This scarce antiquarian book is a facsimile reprint of the old original and may contain some imperfections such as library marks and notations. Because we believe this work is culturally important, we have made it available as part of our commitment for protecting, preserving, and promoting the world's literature in affordable, high quality, modern editions, that are true to their original work.