Title
An Introduction To The Study Of Stellar Structure (Dover Books On Astronomy),New
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In This Monograph A Leading Modern Astrophysicist Explores A Problem Basic To Stellar Dynamics: What Is The Relationship Between Loss Of Energy, Mass, And Radius Of Stars In The Steady State?The Monograph Is Divided Into Two Distinct Parts. In Chapters Iiv, Chandrasekhar Presents The 'Classical' Background Necessary To His Argument: The Laws Of Thermodynamics (From Carathodory'S Rigorous Axiomatic Standpoint), Adiabatic And Polytropic Laws, And The Work Of Ritter, Emden, Kelvin, And Others Who Developed The Applied Mathematics Of Stellar Structure. Chapters Vxii Discuss Modern Results: The Formal Theory Of Radiation, The Equations Of Radiative Equilibrium, The Luminosity Formula, The Theory Of Stellar Envelopes, Gibbs Statistical Mechanics (The Quantum Mechanical Version), White Dwarfs, Etc. The Closing Chapter Outlines Some General Trends In Current Investigations Of The Problem.Appendixes Cover Physical And Astronomical Constants; The Masses Of Light Atoms; The Masses, Luminosities, And Radii Of The Stars, Derived Hydrogen Contents, Central Densities And Central Temperatures, And Tables Of White Dwarf Functions.'Extremely Interesting. It Reaches The Highest Level Of Scientific Merit.' Bulletin, American Mathematical Society.
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- Q: How many pages are in this book? A: This book contains five hundred twelve pages. It's a comprehensive exploration of stellar structure and dynamics.
- Q: What is the binding type of this book? A: The binding type is paperback. This makes it lightweight and portable for easy reading.
- Q: What are the dimensions of this book? A: The dimensions are five point five one inches in length, one point two six inches in width, and eight inches in height. This size is convenient for handling.
- Q: Who is the author of this book? A: The author is Subrahmanyan Chandrasekhar. He was a renowned astrophysicist awarded the Nobel Prize for his work on stellar evolution.
- Q: What genre does this book belong to? A: This book belongs to the astronomy genre. It delves into the principles governing stellar dynamics and structure.
- Q: Is this book suitable for beginners in astrophysics? A: No, this book is not ideal for beginners. It requires a foundational understanding of thermodynamics and stellar dynamics.
- Q: Can I use this book for academic purposes? A: Yes, this book is suitable for academic purposes. It provides in-depth knowledge on stellar structure that can support higher education studies.
- Q: What topics does this book cover? A: This book covers topics like thermodynamics, radiative equilibrium, and stellar envelopes. It also discusses modern astrophysical concepts.
- Q: How should I store this book to keep it in good condition? A: Store this book in a cool, dry place away from direct sunlight. This will help preserve its binding and pages.
- Q: Are there any appendices in this book? A: Yes, there are appendices included. They cover physical and astronomical constants, as well as tables related to white dwarf functions.
- Q: What if I receive a damaged copy of this book? A: If you receive a damaged copy, you can return it for a replacement. Check the retailer’s return policy for specific instructions.
- Q: Is this book safe for young readers? A: No, this book is not specifically designed for young readers. It contains advanced scientific concepts best suited for adults and students.
- Q: Is a glossary included in this book? A: No, a glossary is not specifically mentioned. However, the text is well-explained for those familiar with astrophysics.
- Q: What is the main focus of this book? A: The main focus is on the relationship between energy, mass, and radius of stars in steady state. It explores classical and modern theories.
- Q: Is there a summary of current investigations in this book? A: Yes, the closing chapter outlines general trends in current investigations of stellar structure. It provides insight into ongoing research.
- Q: Can this book be a good reference for research papers? A: Yes, this book can serve as a valuable reference for research papers in astrophysics and related fields. Its scientific merit is highly regarded.