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The Project Gutenberg EBook of Lectures on Stellar Statistics, by Carl Vilhelm Ludvig Charlier This eBook is for the use of anyone anywhere at no cost and with almost no restrictions whatsoever. You may copy it, give it away or re-use it under the terms of the Project Gutenberg License included with this eBook or online at www.gutenberg.org Title: Lectures on Stellar Statistics Author: Carl Vilhelm Ludvig Charlier Release Date: July 27, 2007 [EBook #22157] Language: English Character set encoding: ASCII *** START OF THIS PROJECT GUTENBERG EBOOK LECTURES ON STELLAR STATISTICS *** Produced by Susan Skinner and the Online Distributed Proofreading Team at http://www.pgdp.net (The original copy of this book was generously made available for scanning by the Department of Mathematics at the University of Glasgow.) [Transcriber's Note: This text is intended for users whose text readers cannot use the "real" (unicode/utf-8) version of the file. Characters in the Greek alphabet are represented as follows: [alpha], [beta], [gamma], etc. In the original text, the units h and m, and ordinals th and st were printed as superscripts. For readability, they have not been represented as such in this file. Similarly for the + and - signs when used to describe intermediate stellar colours. Other superscripts are indicated by the carat symbol, ^, and subscripts by an underline, _.] LECTURES ON STELLAR STATISTICS BY C. V. L. CHARLIER SCIENTIA PUBLISHER LUND 1921 HAMBURG 1921 PRINTED BY _LUeTCKE & WULFF_ CHAPTER I. APPARENT ATTRIBUTES OF THE STARS. 1. Our knowledge of the stars is based on their _apparent_ attributes, obtained from the astronomical observations. The object of astronomy is to deduce herefrom the real or _absolute_ attributes of the stars, which are their position in space, their movement, and their physical nature. The apparent attributes of the stars are studied by the aid of their _radiation_. The characteristics of this radiation may be described in different ways, according as the nature of the light is defined. (Undulatory theory, Emission theory.) From the statistical point of view it will be convenient to consider the radiation as consisting of an emanation of small particles from the radiating body (the star). These particles are characterized by certain attributes, which may differ in degree from one particle to another. These attrib
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