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English
Institute of Physics Publishing
23 August 2023
This broad interest text describes how our current understanding of the interiors of the stars came about, beginning in 1870. It starts by discussing the development of our knowledge of the inside of the Sun, and continues on to compare the Sun's and other stars' properties and then discusses how stars form, evolve, and die. The book describes the properties of a variety of stars with special characteristics, and it ends with a discussion of the first stars that formed after the Big Bang. Aiming to show how interesting scientific investigations can encourage young men and women to pursue STEM careers, this book also underscores the role women have played in the development of our understanding.

Key Features

Includes the stories of the historical advances that have led to our current understanding of the nature of the stars Underscores the important roles women have played in the development of this understanding Avoids the use of technical jargon and clearly defines the terms used Identifies some of the key questions that remain unresolved at the time of writing
By:  
Imprint:   Institute of Physics Publishing
Country of Publication:   United Kingdom
Dimensions:   Height: 254mm,  Width: 178mm, 
ISBN:   9780750357920
ISBN 10:   0750357924
Series:   AAS-IOP Astronomy
Pages:   290
Publication Date:  
Audience:   Professional and scholarly ,  Undergraduate
Format:   Hardback
Publisher's Status:   Active
Part I Understanding the Inside of the Sun 1 A Glimpse of the Solar Interior 2 The Sun as a Star 3 The Role of Radiation Inside Stars 4 The Nature of Star Stuff 5 Discovering the Source of Solar Energy 6 Properties of the Matter Inside Stars Part II A Closer Look at the Solar Interior 7 How Our Understanding of the Present Sun Developed 8 Ghost Particles from the Center of the Sun 9 The Sounds of Sunlight Part III From the Sun to the Stars 10 Properties of Main Sequence Stars 11 Where Do Stars Come From? 12 Failed Stars: Brown Dwarfs Part IV Why and How Stars Evolve and Die 13 What Happens When a Low-Mass Star Exhausts Its Nuclear Fuel? 14 How an Intermediate-Mass Star Becomes a White Dwarf 15 White Dwarfs: Fading Embers of Burnt-Out Stars 16 The Evolution of High-Mass Stars and Supernovae 17 Astrophysical Alchemy: Origins of the Chemical Elements 18 Neutron Stars 19 Stellar-Mass Black Holes and Gravitational Waves Part V Stars with Special Characteristics 20 Pulsating Stars 21 Cataclysmic Variables 22 The First Stars Appendix A: Forms of the Hertzsprung–Russell Diagram Appendix B: Some Physical Properties of the Sun Appendix C: Zero-Age Main Sequence Stars Appendix D: Electron Degeneracy Appendix E: Properties of Some Brown Dwarf Stars Appendix F: The Laser Interferometer Gravitational-wave Observatory (LIGO) Appendix G: Zero-Age Main Sequence Models for the First Stars Bibliography

Hugh Van Horn received a Ph.D. from Cornell University and was a faculty member in the Department of Physics and Astronomy at the University of Rochester for almost three decades; he is now a professor emeritus of that University. He also served as the Director of the Division of Astronomical Sciences at the National Science Foundation. Van Horn is now an emeritus member of the American Astronomical Society and a Fellow of the American Association for the Advancement of Science. During his academic career, he published more than 100 technical papers in astrophysics and physics, and he has edited or written several books in these subjects.

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