Methods and technologies of artificial intelligence

 

 

The Structure and Evolution of Stars

Lecture 1. Thermodynamic Equilibrium

Lecture 2. Star Formation. Fragmentation

Lecture 3. Protostars

Lecture 4. Young Stars

Lecture 5. Hydrogen Burning

Lecture 6. Zero-Age Main Sequence (ZAMS) Stars

Lecture 7. Post-AGB Stars

Lecture 8. White Dwarfs

Lecture 9. Evolution of Stars with Masses Greater than 15 Solar Masses

Lecture 10. Evolution of Stars with Masses Greater than 60 Solar Masses

 

Intelligent data processing systems