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.
Price: £67.50
Pages: 186
Publisher: Morgan & Claypool Publishers
Imprint: Morgan & Claypool Publishers
Publication Date:
01 December 2015
Trim Size: 10.00 X 7.00 in
ISBN: 9780750328098
Format: Paperback
BISACs:
SCIENCE / Space Science / Astronomy, Astronomy, space and time
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
