| SES # | TOPICS | KEY DATES |
|---|---|---|
| 1 | Introduction | |
| 2 |
Kepler Problem
Binaries |
|
| 3 |
Stellar Distances
Coordinates Magnitudes |
|
| 4 |
Color-color Diagrams
Spectral/Luminosity Classes |
Problem set 1 due |
| 5 | Saha Equation | |
| 6 |
Radiation
Opacity Radiative Diffusion |
|
| 7 |
Equations of Stellar Structure
Convection |
Problem set 2 due |
| 8 |
Convection (cont.)
Modeling Polytropes Energy Sources |
|
| 9 |
Nuclear Reaction Rates
Hydrogen Burning: pp, CNO |
Problem set 3 due |
| 10 |
H/He Burning
Nucleosynthesis Low-M Stars |
|
| 11 |
Stellar Evolution: Lower Main Sequence
Cluster H-R |
|
| 12 |
S-C Limit
Solar Neutrinos Degenerate Matter |
Problem set 4 due |
| 13 | Midterm Exam | |
| 14 |
Degenerate Matter
Chandra Mass White Dwarfs |
|
| 15 |
White Dwarf Cooling
Intrinsically Variable Stars |
Problem set 5 due |
| 16 | Upper Main Sequence: Evolution of Massive Stars | |
| 17 |
Supernovae
Collapsars GRBs |
Problem set 6 due |
| 18 |
Neutron Stars
Pulsars (Guest Lecturer: David Kaplan) |
Problem set 7 due |
| 19 | Sun as a Star (Guest Lecturer: Justin Kasper) | |
| 20 | Gravitational Radiation (Guest Lecturer: Ryan Lang) | Problem set 8 due |
| 21 |
Close Binaries
Accretion Disks |
|
| 22 |
Cepheid Variables
X-ray Binaries |
Problem set 9 due |
| 23 |
Black Holes
Interstellar Medium Dust Extinction |
|
| 24 |
Star Formation
Jeans Criterion IMF Brown Dwarfs |
Problem set 10 due |
| 25 |
Gas in the Interstellar Medium
Heating and Cooling 21 cm and CO |
|
| 26 |
Shocks
Supernova Remnants |