The Milky Way’s Bulge - From a Hypothesized Blob to a Remarkably Detailed Picture

Explore the complex structure and evolution of the Milky Way's central bulge in this comprehensive lecture by David Nataf of Johns Hopkins University. Delve into the fascinating details of our galaxy's core, which hosts approximately 30% of its stars, including some of the oldest and most metal-rich. Learn about the formation processes of these stars, from early hierarchical collapse to later dynamical processes within the disk. Discover how chemical abundances in stars may influence planet formation and the evolution of life. Gain insights into astronomers' current understanding of the Milky Way's bulge, including its intricate structure and remaining mysteries. Examine various models, observational techniques, and recent discoveries that have contributed to our knowledge of this crucial galactic component. Recorded live at the Space Telescope Science Institute, this talk covers topics such as bulge chemistry, metallicity, galaxy classification, rejected models, and the distribution of stars, providing a thorough overview of our evolving understanding of the Milky Way's central region.

Introduction
Upcoming lectures
Observatory update
Webb delay
Omi
Omi January 2018
PDS 70
News from the Universe
Why the Bulge Matters
Part 1 Chemistry
Part 2 Metallicity
Hubble Tuning Fork Diagram
Bared Spiral Galaxy
Deep Rejected Model
MidInfrared Image
The X
Orbits
Bars
Metalrich Stars
First Evidence
Distributions of Stars
Shortage of Younger Stars
Stars Near the Sun
The Wrinkle
New Analysis
Conclusions