Structure and Evolution of Single Stars: An Introduction
Author:   James MacDonald
Publisher:   Morgan & Claypool Publishers
ISBN:  

9781681740416


Pages:   188
Publication Date:   30 December 2015
Format:   Paperback
Availability:   Available To Order   Availability explained
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Structure and Evolution of Single Stars: An Introduction


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Overview

Structure and Evolution of Single Stars: An introduction is intended for upper-level undergraduates and beginning graduates with a background in physics. Following a brief overview of the background observational material, the basic equations describing the structure and evolution of single stars are derived. The relevant physical processes, which include the equation of state, opacity, nuclear reactions and neutrino losses are then reviewed. Subsequent chapters describe the evolution of low-mass stars from formation to the final white dwarf phase. The final chapter deals with the evolution of massive stars.

Full Product Details

Author:   James MacDonald
Publisher:   Morgan & Claypool Publishers
Imprint:   Morgan & Claypool Publishers
Dimensions:   Width: 17.80cm , Height: 1.00cm , Length: 25.40cm
Weight:   0.333kg
ISBN:  

9781681740416


ISBN 10:   1681740419
Pages:   188
Publication Date:   30 December 2015
Audience:   General/trade ,  General
Format:   Paperback
Publisher's Status:   Active
Availability:   Available To Order   Availability explained
We have confirmation that this item is in stock with the supplier. It will be ordered in for you and dispatched immediately.

Table of Contents

Observational background The equations of stellar structure: mass conservation and hydrostatic equilibrium Energy considerations, the source of the Sun's energy, and energy transport Convective energy transport The equations of stellar evolution and how to solve them Physics of gas and radiation Ionization and recombination The degenerate electron gas Polytropes and the Chandrasekhar mass Opacity Nuclear reactions Neutrino energy loss processes Homology relations Hydrogen main sequence stars Helium main sequence stars The Hayashi line Star formation Evolution on the main sequence and beyond Evolution on the red giant branch Evolution from red giant to white dwarf Evolution of massive stars

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Author Information

The author received his PhD in Astronomy from Cambridge University in 1979. Following postdoctoral positions at the Universities of Sussex and Illinois and Arizona State University, USA he joined the University of Delaware in 1985 where he is now a Professor of Physics and Astronomy. His scientific expertise is the study of the structure and evolution of stars. Recent work has focused on low mass main sequence stars and brown dwarfs. He has published over 80 papers in peer-reviewed journals.

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