Stellar Evolution, Second Edition covers the significant advances in the understanding of birth, life, and death of stars. This book is divided into nine chapters and begins with a description of the characteristics of stars according to their brightness, distance, size, mass, age, and chemical composition. The next chapters deal with the families, structure, and birth of stars. These topics are followed by discussions of the chemical composition and the evolution of main-sequence stars. A chapter focuses on the unique features of the sun as a star, including its evolution, magnetic fields, activity, corona, and neutrinos. Other chapters consider the life histories of individual stars from their birth to their death. The concluding chapter describes the massive changes in Earth's galaxy with time and their observational characteristics. This book will prove useful to astronomers and researchers.
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.
An ideal bridging text for astrophysics and physics majors looking to move on from the introductory texts.
Understanding Stellar Evolution is based on a series of graduate level courses taught at the University of Washington since 2004.
Since its publication, this textbook has come to be considered a classic by both readers and teachers in astrophysics. This study edition is intended for students in astronomy and physics alike.
Sky Atlas 2000.0 , W. Tirion and R. Sinnott , Sky Publishing and Cambridge University Press , 1999 , Massachusetts , USA . Millennium Star Atlas , R. Sinnott and M. Perryman , Sky Publishing , 1999 , Massachusetts , USA .
In this textbook Stars and Stellar Evolution the basic concepts of stellar structure and the main roads of stellar evolution are described.
Physics of Stellar Evolution and Cosmology
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 ...
The recent solar model of Schwarzschild, Howard, & Harm [71] contains an outer convection zone which extends inward only to a temperature close to 1 X 106 0K, which will destroy only deuterium. Hence it is evident that the solar ...
Elements heavier than those , up to nickel , contribute a little , and past there we find only traces . For the most part , the isotopes of the major heavy elements fall along the “ valley of beta - stability " in which Zi / A ; ~ 1/2 .