Lecture

Stellar Orbits: Lindblad Resonances and Collisionless Boltzmann Equation

Description

This lecture covers weak bars, the Lindblad resonances, orbit families in realistic bars, the collisionless Boltzmann equation, the distribution function of stellar systems, solutions of the collisionless Boltzmann equation, stellar orbits in weak rotating bars, resonances, and problematic terms. It also discusses the Miyamoto-Nagai and Plummer potential models, Lindblad resonances, and equilibria of collisionless systems. The instructor emphasizes the importance of self-consistent galaxy models and the assumptions made in studying large stellar systems.

About this result
This page is automatically generated and may contain information that is not correct, complete, up-to-date, or relevant to your search query. The same applies to every other page on this website. Please make sure to verify the information with EPFL's official sources.