Stellar Structure and Evolution

@inproceedings{Kippenhahn1990StellarSA,
  title={Stellar Structure and Evolution},
  author={Rudolf Kippenhahn and Alfred Weigert and Achim Weiss},
  year={1990}
}
This book introduces the theory of the internal structure of stars and their evolution in time. It presents the basic physics of stellar interiors, methods for solving the underlying equations, and the most important results necessary for understanding the wide variety of stellar types and phenomena. The evolution of stars is discussed from their birth through normal evolution to possibly spectacular final stages. Chapters on stellar oscillations and rotation are included. 
View via Publisher
lasp.colorado.edu
1,941 Citations
Highly Influential Citations
163
Background Citations
494
Methods Citations
185
Results Citations
20

Figures from this paper

1,941 Citations

Citation Type

Citation Type

Stellar evolution and modelling stars
In this chapter I give an overall description of the structure and evolution of stars of different masses, and review the main ingredients included in state-of-the-art calculations aiming at…
Introduction to Stellar Evolution
Stellar evolution theory is among the greatest successes of modern astrophysics. It is a powerful tool to interpret many astronomical observations, such as the Colour-Magnitude diagrams of simple and…
Stellar Structure and Evolution: An Introduction
The synthesis of new elements takes place inside stars. How do stars evolve and distribute this creation to the universe at large? This article starts with the observables that the theory of stellar…
The Workings of a Stellar Evolution Code
Models of stellar clusters link the theoretical gravitational N-body problem to the study of real astrophysical systems. Such models require a description of the stars contained within the cluster.…
Modelling the solar interior
The equations of stellar structure and evolution need to be solved to model the interior of the Sun. Modelling the Sun is, however, slightly more complicated than modelling other stars since we have…
The Evolution of Surface Parameters of Rotating Massive Stars
We summarize the present status of the predictions of massive star models for the evolution of their surface properties. After discussing luminosity, temperature and chemical composition, we focus on…
Variational Principles for Stellar Structure
The four equations of stellar structure are reformulated as two alternate pairs of variational principles. Different thermodynamic representations lead to the same hydromechanical equations, but the…
Physical Conditions in the Stellar Interior
This chapter establishes the main equations of the stellar structure, namely, the continuity equation and the hydrostatic equilibrium equation, and gives some estimates of the average density,…
Similarity theory of stellar models and the structure of very massive stars
The similarity theory of stellar models is used to study the properties of very massive stars when all the opacity sources, except the Thomson scattering, can be disregarded. The dimensionless…
Chemical element transport in stellar evolution models
TLDR
The various mechanisms of element transport included in the current generation of stellar evolution calculations are reviewed, how they are implemented, the free parameters and uncertainties involved, the impact on the models and the observational constraints.
...
1
2
3
4
5
...