Cold Streams in the Hot CGM of High Z Galaxies - Han Aung
Offered By: Kavli Institute for Theoretical Physics via YouTube
Course Description
Overview
Explore the dynamics of cold streams in the hot circumgalactic medium (CGM) of high-redshift galaxies in this conference talk. Delve into the properties of massive galaxy halos, CGM observations, and the mechanisms of radiative cooling and deceleration. Examine the survival criterion for cold streams within the halo potential and its implications for galaxy formation. Analyze model predictions and investigate the role of cosmic rays, freefall time scales, and entrainment in shaping these cosmic structures. Gain insights into the co-evolution of the cosmic web and galaxies across cosmic time, as presented at the KITP conference on "The Co-evolution of the Cosmic Web and Galaxies across Cosmic Time."
Syllabus
Introduction
Massive Galaxy
Halos
CGM
Observations
Properties
radiative Cooling
decelerations
survival Criterion
Halo Potential
dissipated power
Implications for galaxy formations
Model predictions
Summary
Cosmic rays
Freefall
Time Scale
Entrainment
Taught by
Kavli Institute for Theoretical Physics
Related Courses
The Gaseous UniverseHubble Space Telescope via YouTube MIGHTEE-HI - The Relation Between the HI Gas in Galaxies and the Cosmic Web - Madalina Tudorache
Kavli Institute for Theoretical Physics via YouTube Formation of Thin and Thick Discs of Galaxies - Sukyoung Yi (Yonsei)
Kavli Institute for Theoretical Physics via YouTube How Cosmological Filaments Reset the Formation of Disc Galaxies - Florent Renaud
Kavli Institute for Theoretical Physics via YouTube The Energy Minimisation Principle - Linking Protohalo Shapes to Anisotropic Infall - Marcello Musso
Kavli Institute for Theoretical Physics via YouTube