YoVDO

Cold Streams in the Hot CGM of High Z Galaxies - Han Aung

Offered By: Kavli Institute for Theoretical Physics via YouTube

Tags

Cosmic Web Courses Cosmology Courses Observational Astronomy Courses Galaxy Formation Courses

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

Introduction to Astronomy
Duke University via Coursera
Galaxies and Cosmology
California Institute of Technology via Coursera
Confronting The Big Questions: Highlights of Modern Astronomy
University of Rochester via Coursera
From the Big Bang to Dark Energy
University of Tokyo via Coursera
Philosophy and the Sciences: Introduction to the Philosophy of Physical Sciences
University of Edinburgh via Coursera