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 |