Explore the fascinating relationship between supermassive black holes and galaxy formation in this hour-long lecture by Mitchell Revalski from the Space Telescope Science Institute. Delve into the powerful winds generated by growing black holes and their role in shaping galaxies, influencing star formation rates, and distributing heavy elements across the universe. Discover recent observations and simulations that shed light on these energetic flows and their impact on galactic evolution. Learn about diverse galaxy populations, active galactic nuclei, ultra-fast outflows, and the intriguing correlations between black hole masses and galaxy characteristics. Gain insights into astronomical spectroscopy, the Hubble Ultra Deep Field, and specific examples like NGC 4 and the Perseus Cluster.
Overview
Syllabus
Space Telescope Public Lecture Series
The Hubble Ultra Deep Field
Tools of the Trade: Astronomical Spectrosco
Galaxies and Supermassive Black Holes SME Face-on Spiral Galaxy
The Milky Way's Supermassive Black Hole
Active Galactic Nuclei (AGN)
Winds and Outflows in Active Galaxies
Ultra-fast Outflows (UFOs)
Black Hole Scaling Relationships
Hubble Space Telescope Spectrum of NGC 4
Outflows in Galaxy Bulges
Galaxy Scale Outflows
Radio Jets in Galaxy Clusters
The Importance of Mass Outflows
The Perseus Cluster - NGC 1275
Taught by
Hubble Space Telescope
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