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A bridge between introductory and advanced technical treatments, this readable and authoritative translation from the French provides an excellent guide to observational astrophysics. Physics students and professionals will appreciate the text's mid-level approach, in which methods of research and observation receive as much attention as results.
Confining his discussion to normal stars, the author examines current methods of stellar photometry and spectroscopy and the main results of research involving star classification and properties. Additional topics include construction of Hertzsprung-Russell diagrams, Yerkes two-dimensional classification, masses and densities of stars, general theories about the constitution of stellar atmospheres and the evolution of stars, and much more. Indispensable for specialists, this volume is also a fine resource for hobbyists and others with some grounding in astronomy wishing to further explore the intricacies of astrophysics.
- Sales Rank: #176157 in Books
- Brand: Brand: Dover Publications
- Published on: 2012-10-17
- Released on: 2012-09-19
- Original language: English
- Number of items: 1
- Dimensions: 8.40" h x .60" w x 5.40" l, .40 pounds
- Binding: Paperback
- 176 pages
- Used Book in Good Condition
About the Author
French astronomer Jean Dufay (1896–1967) computed the altitude of the earth's ozone layer and was named Honorary Director of the Lyon and Haute-Provence observatories. Translator Owen Gingerich is a former Research Professor of Astronomy and the History of Science at Harvard University.
Most helpful customer reviews
13 of 13 people found the following review helpful.
For Anyone Interested, This Book is a Necessity
By Marguerite Abaddonais
For anyone interested in stellar astrophysics, this book gives a very thorough theoretical and practical background in a reasonably short space. It's also written in plain English (which is nice) but doesn't shy away from the math. It's a 'crossover' book that tries to be as useful as a text book but as interesting as a popular science book and I think it succeeds, although I will say it never 'tries too hard' like some PopSci books, and it's a very information-heavy read.
I personally appreciated the Yerkes Classification section, which I had heard about but was nowhere in my astronomy textbook from school.
If you would like to know more about stars and how they work (and how we know how they work), I highly recommend this book.
p.s. For a more history-rich overview of the subject, check out A Concise History of Solar and Stellar Physics
9 of 10 people found the following review helpful.
Introduction to Astrophysics: The Stars
By cortezhill
This work fills a unique position in the literature. It is a concrete, middle-level treatment that devotes as much attention to methods of research and observation as it does to results. Here at last is a book in English which bridges the gap between elementary introductory accounts and advanced technical monographs. In this reliable and readable translation by an eminent American specialist in the field, you will have the best guide to observational astrophysics in the English language.
Linmiting his discussion to normal stars, the author begins with background material covering definitions and problems of measurement through the earth's atmosphere. Current methods of stellar photometry and spectroscopy are described lucidly and precisely: photographic, photoelectric, and thermal measurements; slit and slitless spectrographs; photoelectric and electronic spectrophotometry; etc. He then takes up the main results of research involving the classification and properties of normal stars, giving a general introduction to stellar spectra and their classification and an account of the Harvard scheme of star classes and spectral types.
This material prepares us for the construction of the Hertzsprung-Russell diagrams, which reveal the great families of stars and the two main types od stellar populations, and the Yerkes 2-dimensional classification. Subsequent chapters deal with continuous spectra of the stars, gradients, and color temperatures, spectrophotometric classification of two and three dimensions; diameters and effective temperatures of the stars (including the experiments of Michelson and Pease, the occulation and indirect spectrophotometric methods, principles of interferometric measurements of apparent diameters, etc.); masses and densities of stars; and a discussion of general theories about the constitution of stellar atmospheres and the evolution of stars.
The book provides a firm basis upon which the student will build all is future practical and theoretical work - the background indispensable to any advanced study of the manifold problems of astrophysics. It is also a fine book for hobbyists and others with some grounding in astronomy who want to explore these matters in greater depth than elementary texts allow.
--- excerpt from book's back cover
4 of 4 people found the following review helpful.
Techniques and technology for astronomy
By Daniel N. Lionsden
After reading a few chapters, I realized this was not the book I wanted, although it was very informative. At least the first few chapters were devoted to technology available at the time the book was written. This book is probably great for an instructor who wants to give an overview of how astrophysicists coped with the information obtained by less sophisticated technology.
I can liken this to the transition that took place in the technology employed in the clinical laboratory science between 1925 and the present. Every few years there were advances in lab equipment. Amazing new technologies has replaced the cumbersome flame photometer and single channel chemical analyzers of the 1960s. Automated hematology analyzers have replaced red blood cell count using a microscope and a hemocytometer. Chemistry panels can analyze two or three dozen constituents of the same sample nearly instantaneously once the specimen is sampled.
Similar technological advances have taken place in observatories. Sophisticated, computer assisted equipment can do much more with whatever is being observed than could have been done in 1965.
The reason the book would be useful to the current astrophysics instructor is to give students understanding of the underlying principles of state-of-the-art equipment. They need to know how they results they get from current equipment was gotten. It will help them to know when something is going wrong and how to troubleshoot.
Yes, the book contains many mathematical equations, some of which need to show more minutely how they were derived so the student can understand where the final equations came from. Maybe the author expected readers to know that kind of information prior to reading his book. If this is the case, Dufay did not intend his book to be an introduction to astrophysics any more than Roberts and Caserio meant Basic Principles of Organic Chemistry to be an introduction to organic chemistry.
Seeing the reviews on Francis LeBlanc's An Introduction to Stellar Astrophysics, no doubt it would be more useful to me.
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