Galactic dynamics
Radial Migration
Stars do not stay at the galactocentric radius where they were born. Resonances with the spiral arms and the bar can shuffle a star inward or outward across the disc without heating its orbit, mixing the disc's chemistry over billions of years and complicating any attempt to read history from composition alone.
Galaxy, objects & concepts
Knowledge connections
- Associated withThe Spiral Arms
- Associated withThe Thin Disk
Sources
The primary and reference sources this topic draws on.
- ESOEuropean Southern Observatory
Southern-hemisphere observatory data and imagery (VLT, ALMA partner).