Winter 2018
Physics of stellar interiors and atmospheres
Properties of stars, stellar spectra, radiative transfer, line formation
Stellar structure, stellar evolution
Nucleosynthesis in stars
Stellar oscillations
Seven problem sets, each worth 5% of final grade
MESA stellar evolution model, worth 15% of final grade
Oral midterm, worth 20% of final grade
Written, take-home final exam, worth 30% of final grade
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