Book Description
Donald D. Clayton's Principles of Stellar Evolution and Nucleosynthesis remains the standard work on the subject, a popular textbook for students in astronomy and astrophysics and a rich sourcebook for researchers. The basic principles of physics as they apply to the origin and evolution of stars and physical processes of the stellar interior are thoroughly and systematically set out. Clayton's new preface, which includes commentary and selected references to the recent literature, reviews the most important research carried out since the book's original publication in 1968.
Customer Reviews:
Just perfect!.......2003-01-23
A standard introductory textbook of nuclear astrophysics written by a real expert in a superb style. It has taught nuclear astrophysics to most of us and will teach many more. I keep refering to it all the time. It is my favorite. I warmly recommend it.
A standard reference on stellar structure and evolution.......2000-05-04
"Principles of Stellar Evolution and Nucleosynthesis" is a standard work on stellar structure and evolution. It is clearly written and approachable even by a senior undergraduate. It is a "must" for anyone seriously interested in stellar astrophysics.
Please create an audio adaptation ..........1999-06-02
To the publisher I would appreciate it if the publisher could produce an audio adaptation of this book. I would love to listen to this while I drive to work and to let my 16 month old son listen to it as a bedtime story. Arnold D Veness
Book Description
This text, designed for beginning students of stellar physics, introduces the fundamentals of stellar structure and evolution. In emphasizing the general picture of the life cycles of stars and the physics responsible, it also allows prospective specialists a taste of many of the detailed aspects of this mature discipline. The authors develop a solid foundation in important theory that is often overlooked in typical courses, yet steer clear of extraneous intensive mathematics and physics. Topics include nuclear physics and stellar energy sources, the equation of state of stellar material, phenomenological approaches to convection, and modern numerical techniques for computation of stellar evolution. Keeping pace with recent developments, the authors incorporate important elements such as asteroseismology, and the effects of rotation and magnetic fields. The text contains the source code for two useful programs, ZAMS (for constructing chemically homogeneous zero-age main sequence models) and PULS (to study the seismological properties of the ZAMS models). Some chapters include exercises. The diskette can be used on any computer with a FORTRAN compiler.
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Planetary Nebulae Beyond the Milky Way: Proceedings of the ESO Workshop held at Garching, Germany, 19-21 May, 2004 (ESO Astrophysics Symposia)
Manufacturer: Springer
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Binding: Hardcover
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ASIN: 3540310118 |
Book Description
In the last decade extra-galactic planetary nebulae (PNe) have gained increasing importance. Improved observational capabilities have allowed fainter and fainter PNe to be studied in galaxies well beyond the Milky Way. Planetary nebulae can be detected to at least 30Mpc. They are found in galaxies of all types and also between the galaxies in nearby galaxy clusters. They are valuable as probes, both for providing the velocity of their host stars and also the evolutionary status and relation to the stellar population from which they formed.
This book contains the proceedings of a workshop held at ESO headquarters in Garching in 2004, the first meeting devoted entirely to Extra-galactic Planetary Nebulae. A wide range of topics is covered, from stellar and nebular astrophysics to galactic dynamics and galaxy clusters, making this volume a unique and timely reference of broad astrophysical interest.
Book Description
Studies of stellar formation in galaxies have a profound impact on our understanding of the present and the early universe. The book describes complex physical processes involved in the creation of stars and during their young lives. It illustrates how these processes reveal themselves from radio wavelengths to high energy X-rays and gamma -rays, with special reference towards high energy signatures. Several sections devoted to key analysis techniques demonstrate how modern research in this field is pursued.
Book Description
In this fascinating book, a renowned physicist outlines the discoveries and theories that illuminate the evolution of our world. One of the founders of Big Bang theory, George Gamow employs language that's both scientifically accurate and easy to understand as he traces the development of atomic theory. 1952 edition. 78 illustrations.
Book Description
This text gives a complete and comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The models developed to explain the stability, dynamics and evolution of the stars are presented, and great care is taken to detail the various stages in a star's life. The authors have written a unique text based on their own pioneering work in stellar modeling.
Since its publication, this textbook has come to be considered a classic by readers and teachers in astrophysics. This study edition is meant for students in astronomy and physics alike.
Customer Reviews:
A star's lifetime.......2004-07-30
What happens in the lifetime of a star? This basically is the subject of the book. It describes from basic physical principles where ever possible how a star is formed and how it burns. Kippenhahn shows how inside a star, the gravitational pressure is necessarily balanced by the outgoing radiation and matter pressure.
We see the cycle of how a star burns its hydrogen, synthesising helium in the process. Then, how heavier elements are formed. Finally, whether a star novas or not, depending on its mass.
The Hertzsprung-Russell diagram is shown as a concise way to describe the lifecycle trajectory of a star, over billions of years.
Well suited for physics students.
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Planetary Nebulae: A Study of Late Stages of Stellar Evolution (Astrophysics and Space Science Library)
S.R. Pottasch
Manufacturer: Springer
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ASIN: 9027716722 |
Book Description
Using fundamental physics, the theory of stellar structure and evolution is able to predict how stars are born, how their complex internal structure changes, what nuclear fuel they burn, and their ultimate fate. This undergraduate textbook provides a clear, methodical introduction to the theory of stellar structure and evolution. Starting from general principles and axioms, step-by-step coverage leads students to a global, comprehensive understanding of the subject. Throughout, the book uniquely places emphasis on the basic physical principles governing stellar structure and evolution. All processes are explained in clear and simple terms with all the necessary mathematics included. Exercises and their full solutions allow students to test their understanding. This book requires only a basic background in physics and mathematics and assumes no prior knowledge of astronomy. It provides a stimulating introduction for undergraduates in astronomy, physics, planetary science and applied mathematics taking a course on the physics of stars.
Customer Reviews:
alright........2006-11-06
the book is alright, the 2nd half is just qualitative discussion, most of which you've proabably already heard. the first half is the best, gives all of the equations of stellar structure, but has some really annoying convensions -- it's in MKS units, and it denotes luminosity by 'F' which really threw me off at first. hmmm, the conversation is a little uninspiring too...
Nice book that cover a lot of topics.......2006-10-19
This is a nice book that covers a lot of astrophysical concepts. The level of detail is fair for a first introduction into the subject and the style is easy to follow. However, the different topics are introduced one after the other without a clear motivation. This makes the book a bit confusing.
Excellent book for beginners.......2004-05-16
A truly excellent introductory book. It has worked problems at the back and actually has an index that allows you to find anything you need for reference. I actually used this book more than Padmanabhan's books for my graduate course, because Prialnik explains things very well.
This book should be the basis of any undergraduate stellar astrophysics course.
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Evolution of Stars and Stellar Populations
Maurizio Salaris , and
Santi Cassisi
Manufacturer: Wiley
ProductGroup: Book
Binding: Paperback
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ASIN: 0470092203 |
Book Description
Evolution of Stars and Stellar Populations is a comprehensive presentation of the theory of stellar evolution and its application to the study of stellar populations in galaxies. Taking a unique approach to the subject, this self-contained text introduces first the theory of stellar evolution in a clear and accessible manner, with particular emphasis placed on explaining the evolution with time of observable stellar properties, such as luminosities and surface chemical abundances. This is followed by a detailed presentation and discussion of a broad range of related techniques, that are widely applied by researchers in the field to investigate the formation and evolution of galaxies.
This book will be invaluable for undergraduates and graduate students in astronomy and astrophysics, and will also be of interest to researchers working in the field of Galactic, extragalactic astronomy and cosmology.
* comprehensive presentation of stellar evolution theory
* introduces the concept of stellar population and describes "stellar population synthesis" methods to study ages and star formation histories of star clusters and galaxies.
* presents stellar evolution as a tool for investigating the evolution of galaxies and of the universe in general.
Download Description
Evolution of Stars and Stellar Populations is a comprehensive presentation of the theory of stellar evolution and its application to the study of stellar populations in galaxies. Taking a unique approach to the subject, this self-contained text introduces first the theory of stellar evolution in a clear and accessible manner, with particular emphasis placed on explaining the evolution with time of observable stellar properties, such as luminosities and surface chemical abundances. This is followed by a detailed presentation and discussion of a broad range of related techniques, that are widely applied by researchers in the field to investigate the formation and evolution of galaxies. This book will be invaluable for undergraduates and graduate students in astronomy and astrophysics, and will also be of interest to researchers working in the field of Galactic, extragalactic astronomy and cosmology. comprehensive presentation of stellar evolution theory. introduces the concept of stellar population and describes ""stellar population synthesis"" methods to study ages and star formation histories of star clusters and galaxies. presents stellar evolution as a tool for investigating the evolution of galaxies and of the universe in general.
Book Description
Stellar evolution - the birth, development and death of stars - is central to our current understanding of astronomy. This area of astrophysics is often portrayed as being difficult and mathematical, but Mike Inglis brings it to life in a unique way, combining a step-by-step introduction with suggestions for making practical observations of stars at different stages in their evolution. Every amateur astronomer - regardless of their current level of knowledge - will find this book fascinating and informative.
Customer Reviews:
Potentially Good Book; Copyediting at its worst.......2003-09-23
Observer's Guide to Stellar Evolution
Review 1003
Book Review: `Observer's Guide to Stellar Evolution'
By Richard Tihany
"The Observer's Guide to Stellar Evolution" by Mike Inglis (Springer-Verlag) can be used as a quick reference to a few hundred commonly observed astronomical objects. The author also provides a comprehensive explanation of the basics of astrophysics, using the objects as illustrations of the concepts he presents within the text.
Inglis meticulously discusses in great detail the methods of measurement of such essential astronomical details as distances and the use of spectral analysis of starlight to determine stars' composition and relationship to other objects.
We are taken from the formation of protostars in the interstellar medium to the actual birth of a star, at the point when pressure and temperature increase enough to start the core's hydrogen-fusion reaction, producing first helium and then all other elements, known as metals to astronomers.
The author imparts one of the most important concepts of astronomy in his handling of the Hertzsprung-Russell Diagram, a compilation of research named in 1911 for Danish astronomer Ejnar Hertzsprung and, in 1913, for American astronomer Henry Norris Russell. He repeatedly approaches the H-R diagram from several avenues, including measurements of the radii of stars and consideration of every possible facet of a star's genesis, life and death.
Inglis deals with the H-R diagram more effectively than many authors by the deftness with which he reapproaches the subject time after time. Rather than creating the impression of being overbearing and too repetitive, Inglis increases the reader's understanding of the H-R diagram's importance to the concepts under consideration. His explanation of the crux of the H-R diagram, the diagonal band of stars know collectively as the "main sequence," is key to any further understanding of astronomy, for these stars comprise 90% of all visible stars.
Inglis' explanation of the "proton-proton chain," the series of nuclear
reactions by which four hydrogen atoms interact at extremely high temperatures to form one helium atom, is the best I've read. His lucid description of helium burning, which results in the creation of carbon and oxygen, couldn't be clearer. The next main event in the sequence, the "helium flash," only happens in low-mass stars but is best described as spectacular: energy output about 100 times greater than the entire Milky Way. The temperature of the star's core at this point can reach 300 million K.
Due deference to the mathematically-challenged is provided by Inglis' decision to keep nearly all formulas and computations separate from the text in shaded boxes scattered throughout the book. The book's diagrams are well-done and informative. I intend to plan some observing sessions in the near future by referring to the object descriptions.
Notably missing is an effective and comprehensive glossary. This necessitates frequent use of the index, a poor substitute.
While this book is the product of a talented astronomer, it reveals the worst example of copyediting I've seen in years. The reader is forced to reread many sentences and to guess their meaning. In fact, only a determined reader is likely to finish the book.
The author knows better than to say (page 36), "It is easier to have an idea of a star if we say it is about 10 times as hotter (sic) than the Sun..." Or, (page 73) "...they can in affect (sic) sweep away the residual gas and dust clouds...." On page 101, Inglis tells us that a star cluster "...can vary from a few dozen light years to about 70 light years across...." (70 is a few dozen.) On page
117, he states, "The mechanisms by which provides the `triggers' for star formation have three very disparate origins..."(By which what provides the
triggers?) I was repeatedly left with the impression that Springer is selling a fairly thin paperback for $44.95 which could be more aptly identified as a rough draft than a book. However, the factual content is valuable despite the nearly fatal defects. This impression is largely due to my knowledge of astronomy before venturing into this prematurely-published minefield. Had I paid for the book rather than been provided a review copy, I would have been tempted to return it.
The current edition of this book could be the makings of a rather good book if Inglis, his editor and his publisher decide to complete the project.
Don't be Afraid of Math.......2003-08-14
My definition of a good Scientific American article is that an intelligent person outside the specialty can understand it. Mike Inglis definitely passes this test! As a mechanical engineer I especially appreciate the basic math that applies to magnitudes, distances, and stellar sizes. The H-R diagram is covered from many angles in a more logical, understandable format than I have ever read. I will definitely wear out this book going over the good sections time after time (sometimes under red light!)
Chris Norris
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- Reflecting Telescope Optics I: Basic Design Theory and its Historical Development (Astronomy and Astrophysics Library)
- Resources of the Earth: Origin, Use, and Environmental Impact (3rd Edition)
- Rocket Propulsion Elements, 7th Edition
- Rocket Propulsion Elements, 7th Edition
- Sams Teach Yourself Macromedia Flash 8 in 24 Hours (Sams Teach Yourself)
- Sandworms of Dune
- Son of the Morning Star
- Standing in the Spaces: Essays on Clinical Process, Trauma, and Dissociation
- Stephen Hawking's Universe: The Cosmos Explained
- Superconductivity: Part 2 (In Two Parts) (Superconductivity)
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