Completed
Intro
Class Central Classrooms beta
YouTube videos curated by Class Central.
Classroom Contents
Multi-Phase Gas in and Around Young, Star-Forming Molecular Clouds - Stefanie Walch-Gassner
Automatically move to the next video in the Classroom when playback concludes
- 1 Intro
- 2 Multi-phase ISM and molecular cloud formation
- 3 Multi-phase model of the atomic ISM
- 4 A quick word on Cosmic Rays... Outflows become cooler and smoother
- 5 The SILCC project (www.astro.uni-koeln.de/silcc): Typical mass distribution in the multi-phase ISM in a star forming palactic disk
- 6 Position of Supernovae with respect to dense gas changes the ISM phase distribution!
- 7 Momentum input: Stellar winds vs. ionizing radiation
- 8 SILCC-Zoom: MHD simulation + star formation & radiative feedback
- 9 Feedback pushes gas into the thermally unstable regime
- 10 Stellar feedback processes determine the multi-phase ISM structure
- 11 Mass loading and energy loading of outflowing gas
