Astro 3104 💎 ⭐

The first third of ASTRO 3104 focuses on the question: Why does the Milky Way look and move the way it does?

Students usually need a solid foundation in: astro 3104

Consolidates stator end windings to protect against mechanical forces. The first third of ASTRO 3104 focuses on

Almost every version of 3104 includes a final project where you write a simple 1D stellar model. You will watch a 1 solar-mass star evolve for 10 Gyr in 30 seconds of code. It is mesmerizing. You will watch a 1 solar-mass star evolve

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You will be handed a histogram of [Fe/H] for 10,000 stars and asked: "How many distinct populations do you see?" The answer is rarely obvious due to observational errors and overlapping distributions.

: Work through every step of the potential derivation for a Kuzmin disk or a Miyamoto-Nagai potential. Write out Poisson’s equation in cylindrical coordinates ((R, \phi, z)) until it becomes intuitive.