The Observation And Analysis Of Stellar Photospheres
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Author | : David F. Gray |
Publisher | : Cambridge University Press |
Total Pages | : 560 |
Release | : 2005-11-17 |
Genre | : Science |
ISBN | : 9780521851862 |
Third edition textbook for use on advanced courses on stellar physics.
Author | : David F. Gray |
Publisher | : Cambridge University Press |
Total Pages | : 476 |
Release | : 1992-06-04 |
Genre | : Science |
ISBN | : 9780521408684 |
Describes the equipment, observational techniques and analysis used in the investigation of stellar photospheres.
Author | : David F. Gray |
Publisher | : Cambridge University Press |
Total Pages | : 536 |
Release | : 2021-12-16 |
Genre | : Science |
ISBN | : 1009085417 |
This textbook describes the equipment, observational techniques, and analysis used in the investigation of stellar photospheres. Now in its fourth edition, the text has been thoroughly updated and revised to be more accessible to students. New figures have been added to illustrate key concepts, while diagrams have been redrawn and refreshed throughout. The book starts by developing the tools of analysis, and then demonstrates how they can be applied. Topics covered include radiation transfer, models of stellar photospheres, spectroscopic equipment, how to observe stellar spectra, and techniques for measuring stellar temperatures, radii, surface gravities, chemical composition, velocity fields, and rotation rates. Up-to-date results for real stars are included. Written for starting graduate students or advanced undergraduates, this textbook also includes a wealth of reference material useful to researchers. eBook formats include color imagery while print formats are greyscale only; a wide selection of the color images are available online.
Author | : William Kenneth Rose |
Publisher | : Cambridge University Press |
Total Pages | : 502 |
Release | : 1998-04-16 |
Genre | : Science |
ISBN | : 9780521588331 |
This advanced 1998 textbook on stellar astrophysics provides a comprehensive and self-contained introduction for graduate students.
Author | : Michel Cassé |
Publisher | : Cambridge University Press |
Total Pages | : 266 |
Release | : 2003-08-07 |
Genre | : Nature |
ISBN | : 9780521821827 |
Author | : Marc F. M. Trypsteen |
Publisher | : Cambridge University Press |
Total Pages | : 167 |
Release | : 2017-07-20 |
Genre | : Nature |
ISBN | : 1107166187 |
This accessible guide presents the astrophysical concepts behind astronomical spectroscopy, covering both theoretical and practical elements. Suitable for anyone with only a little background knowledge and access to amateur-level equipment, it will help you understand and practise the scientifically important and growing field of amateur astronomy.
Author | : David F. Gray |
Publisher | : Cambridge University Press |
Total Pages | : 535 |
Release | : 2021-12-16 |
Genre | : Science |
ISBN | : 1009078011 |
A rigorous, engaging advanced textbook on stellar atmospheres: from equipment and observational techniques to analysis and applications.
Author | : Wolfgang Steinicke |
Publisher | : BoD – Books on Demand |
Total Pages | : 162 |
Release | : 2019-05-23 |
Genre | : Science |
ISBN | : 3749451788 |
Nebulae, star clusters, and galaxies are outside our solar system. They belong to the 'deep sky' and lead the observer to great distances and at the same time the view goes far into the past. The light of the most distant galaxies took billions of years to reach us. No less fascinating is our home galaxy, the Milky Way, offering many bright nebulae and star clusters. The book covers three important topics related to deep-sky objects: history, astrophysics, and observation. When beginners observe an object visually, not knowing anything about it, they will only perceive a faint spot of light - nothing really exciting. So, to get the right 'cosmic' feeling, the view should be enriched with stories about the object's discovery, distance, physical nature, or evolution. Supplied with this kind of information, deep-sky observing becomes a fascinating activity - braving the cold and darkness. Over time, advanced fields such as observation techniques or astrophotography come into play. The book informs the reader about all these topics and offers a comprehensive collection of interesting targets.
Author | : Ivan Hubeny |
Publisher | : Princeton University Press |
Total Pages | : 944 |
Release | : 2014-10-26 |
Genre | : Science |
ISBN | : 0691163294 |
The most authoritative synthesis of the quantitative spectroscopic analysis of stellar atmospheres This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the observable outer layers of stars and similar objects. Written by two leading researchers in the field, it presents a comprehensive account of both the physical foundations and numerical methods of such analyses. The book is ideal for astronomers who want to acquire deeper insight into the physical foundations of the theory of stellar atmospheres, or who want to learn about modern computational techniques for treating radiative transfer in non-equilibrium situations. It can also serve as a rigorous yet accessible introduction to the discipline for graduate students. Provides a comprehensive, up-to-date account of the field Covers computational methods as well as the underlying physics Serves as an ideal reference book for researchers and a rigorous yet accessible textbook for graduate students An online illustration package is available to professors at press.princeton.edu
Author | : Erika Böhm-Vitense |
Publisher | : Cambridge University Press |
Total Pages | : 308 |
Release | : 1989 |
Genre | : Science |
ISBN | : 9780521348713 |
This book is the final one in a series of three texts which together provide a modern, complete and authoritative account of our present knowledge of the stars. It discusses the internal structure and the evolution of stars, and is completely self-contained. There is an emphasis on the basic physics governing stellar structure and the basic ideas on which our understanding of stellar structure is based. The book also provides a comprehensive discussion of stellar evolution. Careful comparison is made between theory and observation, and the author has thus provided a lucid and balanced introductory text for the student. As for volumes 1 and 2, volume 3 is self-contained and can be used as an independent textbook. The author has not only taught but has also published many original papers in this subject. Her clear and readable style should make this text a first choice for undergraduate and beginning graduate students taking courses in astronomy and particularly in stellar astrophysics.