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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
Explosive Stellar Events
Core-Collapse Supernovae
Type II Supernovae
Hydrogen-Rich Spectra
Red Supergiant Progenitors
Core Collapse Mechanism
Type Ib Supernovae
Hydrogen-Poor Spectra
Helium-Rich Composition
Wolf-Rayet Progenitors
Type Ic Supernovae
Hydrogen and Helium Poor
Stripped Envelope Stars
Broad-Line Events
Explosion Mechanism
Iron Core Collapse
Neutron Star Formation
Neutrino-Driven Explosion
Shock Revival
Observational Properties
Light Curves
Spectral Evolution
Energy Output
Remnant Formation
Thermonuclear Supernovae
Type Ia Supernovae
White Dwarf Progenitors
Binary Evolution
Chandrasekhar Mass
Thermonuclear Runaway
Explosion Models
Deflagration
Detonation
Delayed Detonation
Standard Candle Properties
Peak Luminosity
Light Curve Shape
Cosmological Applications
Progenitor Systems
Single Degenerate
Double Degenerate
Observational Constraints
Supernova Remnants
Shock Wave Propagation
Sedov-Taylor Phase
Radiative Phase
Supernova Remnant Types
Shell-Type SNRs
Plerions
Composite SNRs
Interaction with ISM
Shock Heating
Cosmic Ray Acceleration
Chemical Enrichment
Other Explosive Events
Hypernovae
Extremely Energetic Explosions
Gamma-Ray Burst Connection
Pair-Instability Supernovae
Very Massive Star Deaths
Complete Disruption
Electron-Capture Supernovae
Super-AGB Star Explosions
Intermediate Mass Range
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7. Stellar Death and Remnants
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9. Variable Stars