Editorial Review:
The Physics of Stars, Second Edition, is a concise introduction to the properties of stellar interiors and consequently the structure and evolution of stars. Strongly emphasising the basic physics, simple and uncomplicated theoretical models are used to illustrate clearly the connections between fundamental physics and stellar properties. This text does not intend to be encyclopaedic, rather it tends to focus on the most interesting and important aspects of stellar structure, evolution and nucleosynthesis. In the Second Edition, a new chapter on Helioseismology has been added, along with a list of physical constants and extra student problems. There is also new material on the Hertztsprung-Russell diagram, as well as a general updating of the entire text. It includes numerous problems at the end of each chapter aimed at both testing and extending student's knowledge. Cached date: AWS Called=true
You may also be interested in these products:
These categories may also be of interest to you:
Customer Reviews
Average Customer Rating: 
Very Good 2007-06-06 Just finished using this book as part of an Astrophysics corse in University College Cork. It has a straight forward layout and with lucid explanations of the essential topics.
Clear and Concise presentation 2002-12-01 This book is one of the set texts for the Third Level Open University course, "The Energetic Universe" and provides a good introduction to the subject of Astrophysics. Drawing upon a number of basic principles within Physics, such as heat transfer, the fundamental properties of matter, radiation physics, thermonuclear reactions, and nucleosynthesis, the author applies them to explain the birth, evolution and death of stars. What I like about this book is that the emphasis is on the basic physical principles, bringing them together by means of well explained and simple theoretical models, and then applying them to the high energy systems of stellar structure. The Maths is kept to the necessary minimum, and several "rough" calculations are given to show the relevance of the models to observation. The problems at the end of the chapters together with hints help to underpin the physical concepts covered. There is at the end of the book also a useful bibliography of other relevant reading.
|
|