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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
Post-Main-Sequence Evolution
Low-Mass Stellar Evolution
Hydrogen Shell Burning Phase
Core Hydrogen Exhaustion
Shell Source Ignition
Structural Readjustment
Red Giant Branch
Core Contraction
Envelope Expansion
Convective Envelope
First Dredge-Up
Helium Flash
Degenerate Core Conditions
Triple-Alpha Process
Flash Characteristics
Core Helium Ignition
Horizontal Branch Phase
Core Helium Burning
Hydrogen Shell Burning
Stellar Structure
RR Lyrae Instability
Asymptotic Giant Branch
Double Shell Burning
Thermal Pulses
Third Dredge-Up
s-Process Nucleosynthesis
Planetary Nebula Formation
Mass Loss Enhancement
Envelope Ejection
Central Star Evolution
Nebular Ionization
Intermediate-Mass Stellar Evolution
Post-Main-Sequence Tracks
Blue Loop Evolution
Cepheid Instability Strip
Multiple Crossings
Advanced Nuclear Burning
Carbon Burning
Neon Burning
Oxygen Burning
Mass Loss Effects
Stellar Winds
Evolutionary Consequences
High-Mass Stellar Evolution
Rapid Evolution
Short Lifetimes
Massive Star Tracks
Advanced Burning Stages
Helium Burning
Carbon Burning
Neon Burning
Oxygen Burning
Silicon Burning
Onion-Shell Structure
Layered Burning Shells
Core Composition Evolution
Convective Zones
Iron Core Formation
Silicon Burning Products
Nuclear Statistical Equilibrium
Core Mass Growth
Chandrasekhar Mass Approach
Pre-Supernova Evolution
Core Instability
Neutrino Losses
Final Moments
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5. Stellar Evolution: Main Sequence Phase
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7. Stellar Death and Remnants