Table of Contents
Introduction
to Stellar Evolution
Outline
Stellar Structure
Equations (1)
Stellar Structure
Equations (2)
Physical input for stellar
models
Assumptions and commonly
omitted physics
Constraints for solar and
stellar models
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Why does a star shine?
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Nuclear energy generation
rates
Interior structure of
main-sequence stars
What happens to a star
like the Sun?
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The Future of the Sun (1)
The Future of the Sun (2)
The Future of the Sun (3)
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What happens to a star
only 1/10 the mass of the Sun?
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What happens to a star 15
times as massive as the Sun?
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Mass Breakpoints
Star formation
considerations (1)
Star formation
considerations (2)
Number of stars of
different masses
Stellar Recycling
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