Astrophysical Dynamics
Lecture, three hours. Orbital dynamics: two-body problem, three-body problem, resonances, tides, migration. Galactic potentials. Milky Way structure and observed properties of galaxies. Collisionless Boltzmann equation and relaxation processes. Stability of stellar systems. Spiral structure. Letter grading.
Review Summary
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Enrollment Progress
Jul 13, 4 PM PDT
LEC 1: 0/0 seats taken (Canceled)
Course
Previous Grades
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