Useful Links
Physics
Astrophysics and Cosmology
Stellar Astronomy and Astrophysics
1. Introduction to Stellar Astrophysics
2. Measurable Properties of Stars
3. Stellar Structure and Atmospheres
4. Star Formation
5. Stellar Evolution: Main Sequence Phase
6. Post-Main-Sequence Evolution
7. Stellar Death and Remnants
8. Explosive Stellar Events
9. Variable Stars
10. Binary and Multiple Star Systems
11. Stellar Nucleosynthesis and Chemical Evolution
Stellar Evolution: Main Sequence Phase
Zero-Age Main Sequence
Arrival Conditions
Pre-Main-Sequence Contraction
Onset of Hydrogen Burning
ZAMS Properties
Nuclear Fusion Processes
Hydrogen Burning
Proton-Proton Chain
PP-I Chain
PP-II Chain
PP-III Chain
CNO Cycle
CN Cycle
NO Cycle
Temperature Dependence
Core Conditions
Temperature Requirements
Pressure Requirements
Quantum Tunneling
Gamow Peak
Main Sequence Structure
Mass-Dependent Structure
Low-Mass Stars
Intermediate-Mass Stars
High-Mass Stars
Convective Cores
Convective Core Mass
Core Hydrogen Depletion
Semiconvection
Radiative Envelopes
Energy Transport
Opacity Effects
Main Sequence Evolution
Compositional Changes
Hydrogen Depletion
Helium Accumulation
Mean Molecular Weight
Structural Changes
Core Contraction
Envelope Expansion
Luminosity Evolution
Evolutionary Timescales
Nuclear Timescale
Main Sequence Lifetime
Mass-Lifetime Relation
Mass-Dependent Properties
Mass-Luminosity Relation
Theoretical Basis
Observational Confirmation
Mass Range Validity
Mass-Radius Relation
Structural Dependence
Equation of State Effects
Mass-Temperature Relation
Core Temperature
Effective Temperature
Previous
4. Star Formation
Go to top
Next
6. Post-Main-Sequence Evolution