Fall 2019
Thermodynamics, equation of state, convection, opacity, radiative transfer, stellar atmospheres, nuclear reactions, and stellar models.
Evolution of low- and high-mass stars, supernovae, and binary stars.
Six problem sets, worth 50% of final grade
Class project, worth 15% of final grade
Oral midterm, worth 10% of final grade
Written, take-home final exam, worth 25% of final grade
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