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MIGHTEE-HI - The Relation Between the HI Gas in Galaxies and the Cosmic Web - Madalina Tudorache

Offered By: Kavli Institute for Theoretical Physics via YouTube

Tags

Cosmic Web Courses Cosmology Courses Observational Astronomy Courses Galaxy Formation Courses Radio Telescopes Courses

Course Description

Overview

Explore the relationship between neutral hydrogen gas in galaxies and the cosmic web in this 27-minute conference talk from the "Co-evolution of the Cosmic Web and Galaxies across Cosmic Time" conference. Delve into the MIGHTEE-HI survey, examining how the cosmic web influences galaxy formation and evolution. Discover the observational techniques, data sources, and parameters used to study HI alignment and distribution. Learn about the limitations of current radio telescopes and the challenges in detecting the spin transition of neutral hydrogen. Gain insights into the barrier mass concept and its implications for galaxy formation. Conclude with key takeaways and potential future research directions in this fascinating field of astrophysics.

Syllabus

Introduction
How does this affect the galaxies
Network
Neutral Hydrogen
H1 Alignment
Data Source
Field Selection
Parameters
Radio telescopes
Mighty Survey
Radio galaxies
Limitations
Spin Transition
Barrier Mass
Summary
Takeaway
Future work
Questions


Taught by

Kavli Institute for Theoretical Physics

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