SES # | TOPICS |
---|---|
L1 | Introduction: What is a Galaxy? |
L2 | How Do You Build a Galaxy? |
L3 | How are Galaxies Described? |
L4 | Gravitational Potentials: General Results |
L5 | Interesting and Special Cases |
L6 | Orbits in Spherical Potentials and Integrals |
L7 | Orbits in Axisymmetric Potentials Epicyclic Approximation |
L8 | Equilibria of Stellar Systems Boltzmann Equation |
L9 | Jeans' Equations in Spherical Coordinates |
L10 | Jeans' Equations Applied Jeans' Theorem |
L11 | Stability: Jeans Mass and Spiral Structure |
L12 | Gravitational Mirages (aka lenses) via Fermat's Principle |
L13 | Applied Gravitational Lensing |
L14 | Weak Lensing |
L15 | Clusters of Galaxies |
L16 | Physics in Clusters of Galaxies |
L17 | The Sunyaev-Zeldovich Effect |
L18 | Cosmology: Recent History and a Serviceable Newtonian Model |
L19 | The Spherical Model |
E1 | In-class Exam |
L20 | Recombination |
L21 | From Fields to Objects: The Press-Schecter Recipe |
L22 | Adding GR to Cosmology |
L23 | Distances in Cosmology |
L24 | Cosmological Parameters |
L25 | Growing Modes in Expanding Universes: Jeans Redux |
L26 | Growing Modes: Radiation Dominated and Non-baryonic Universes |
L27 | Statistical Measures of Cosmic Structure |
L28 | The Cosmic Microwave Background and its Fluctuations |
L29 | Cosmological Helium Production |
L30 | Details of Helium Production |
L31 | Absorbers along Quasar Lines of Sight |
L32 | Active Galactic Nuclei |
L33 | The Black Hole Paradigm for AGN |
L34 | Accretion Disks |
L35 | Superluminality and Jets |
L36 | Extragalactic Sky Brightness: Present and Past Superposed |
L37 | Bonus Lecture #1 |
L38 | Bonus Lecture #2 |
E2 | Three-hour Final Exam |