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Revising topics and results to include the latest research, this updated third edition describes the equipment, observational techniques, and analysis used to investigate stellar photospheres. Topics covered include radiation transfer, models of stellar photospheres, spectroscopic equipment, observing stellar spectra, and techniques for measuring stellar characteristics. The comprehensive textbook is ideal for advanced students of stellar physics. Each chapter contains exercises, and useful real star data and primary references can be found throughout.
- Sales Rank: #4059615 in Books
- Published on: 2005-11-28
- Original language: English
- Number of items: 1
- Dimensions: 9.72" h x 1.14" w x 6.85" l, 2.70 pounds
- Binding: Hardcover
- 550 pages
Review
"...this new edition sustains the strenths of its predecessors while introducing new material, including (for the first time) exercises that enhance its usefulness as source material for lecture courses...all the expected standard topics are well covered, with a clarity that readily betrays the author's deep familiarity with, and understanding of, both the central physics and the empirical practice. Any atypical content and emphasis also reflects this first-hand command of the material, and sets the book apart from (and above) a number of others that attempt to cover broadly similar ground...accessible at undergraduate level, and with enough depth (and referencing to primary sources) to make it useful for the research scientist. Recommended to all with interests in these areas." - The Observatory, Ian D. Howarth
About the Author
David F. Gray is Director of the Elginfield Observatory and Professor of Astronomy at the University of Western Ontario, London, Canada.
Most helpful customer reviews
0 of 1 people found the following review helpful.
Five Stars
By S. Sousa
Spectroscopy related studies: must have book...
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By Carmelo
Excellent
1 of 1 people found the following review helpful.
Aimed at the Oberver, Not the Theoretical Aspects
By John Matlock
This book is aimed at the advanced undergraduate or graduate student in astronomy or astrophysics. It is well suited for use as a university text, probably for a one year course. It also includes enough matherial to be useful to research scientists who may have specialized in other areas. The orientation of the book is more to the observer and analyzer of steller atmospheres rather than the theoretical approach.
In my opinion the student should have enough of a background in astronomy to at least understand the concept of spectrum lines. And math through Fourier transforms -- Chapter two of this book covers Fourier transforms, but twenty-five pages isn't quite enough to provide the understanding that I believe is needed for the rest of the book, or indeed for the questions that end Chapter 2.
This is the third edition of the book. It is updated to include the recent discoveries in both observations and the analytical tools that have been developed. To a lessor extent, some areas of the book have been revised to follow suggestions made by users of the previous editions.
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