https://bib.cozmix.cloud/files/original/858115b814e475c2bcde2a337d646f98.jpg 512916f431e05ba462866eb97e1f41f1 Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Sterren Boek Een boek. ISBN International Standard Book Number 521255481 Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Identifier An unambiguous reference to the resource within a given context STE0535 Creator An entity primarily responsible for making the resource J. B. Hearnshaw Title A name given to the resource The Analysis of Starlight: One Hundred and Fifty Years of Astronomical Spectroscopy Publisher An entity responsible for making the resource available Cambridge University Press Date A point or period of time associated with an event in the lifecycle of the resource 30 January, 1987 Description An account of the resource This book presents a detailed pedagogical account of the equation of state and its applications in several important and fast growing topics in theoretical physics, chemistry and engineering. This book is the storv of the analysis of starlight by astronomical spectroscopy. It describes the development of the subject from the time of Joseph Fraunhofer, who, in 1814, used a telescope-mounted prism to observe the spectral light emitted from several bright stars. He discovered that light was missing at certain colours (wavelengths) in the starlight, and these so-called spectral lines were subsequently shown to hold clues to the nature of the stars themselves. The book explains how the classification of stars using their line spectra developed into a major branch of astronomy whilst new methods in astrophysics made possible the approximate quantitative analysis of spectral lines in the 1920s and 1930s. After the Second World War these techniques were considerably improved when computers were programmed to model the structure of the outer layers of stars. Basic concepts in spectroscopy and spectral analysis are also covered and. finally. Dr Hearnshaw comments on the stellar spectroscopy of some individual star. Language A language of the resource nothing Format The file format, physical medium, or dimensions of the resource Hardcover