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1
Introduction
2
What makes UCLA special
3
The Short Shield Radius
4
Supermassive Black Holes
5
Primadonnas
6
Center of the Galaxy
7
History Lesson
8
Campaign Promise 1
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Campaign Promise 2
10
Airflow
11
The Atmosphere
12
Hubble Space Telescope
13
Keck Telescope
14
Simple Technique
15
Early Technique
16
Adaptive Optic System
17
Real Data
18
Advanced Evidence
19
New Technologies
20
Tidal Forces
21
Paradox of Youth
22
Pink Objects
23
Binary Stars
24
The 30 Meter Telescope
Description:
Explore groundbreaking developments in the study of supermassive black holes through this captivating lecture by Nobel laureate Dr. Andrea M. Ghez. Delve into the UCLA Galactic Center Group's two-decade journey of high-resolution imaging that transformed the existence of a supermassive black hole at our galaxy's center from possibility to certainty. Discover how stellar orbit measurements around a galactic nucleus provided compelling evidence for these exotic cosmic entities. Uncover unexpected findings in the black hole's environment, including young stars in unlikely locations, a scarcity of old stars, and a mysterious new class of objects. Gain insights into black hole growth, their role in galactic evolution, and recent observations shedding light on gravity's behavior near these massive cosmic phenomena. Learn about cutting-edge high-resolution imaging technologies and their impact on black hole research, as Dr. Ghez shares her expertise in observational astrophysics and the fascinating discoveries made at the Galactic Center. Read more

From the Possibility to the Certainty of a Supermassive Black Hole - IPAM UCLA

Institute for Pure & Applied Mathematics (IPAM)
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