Radial migration — where it appears
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
An arm that is undone by the work it does
A spiral pattern takes angular momentum from the inner disc and delivers it to the outer, which lets mass move inwards without violating anything. It is paid for in random motion, and a disc with too much random motion cannot carry a wave — so the pattern destroys the conditions it needs to exist.
A gradient the old stars have walked away from
The gas in a disc galaxy is richer in metals near the centre than at the edge, by about six-hundredths of a dex per kiloparsec in the Milky Way. Two ingredients of disc growth make that slope, a disc that grows from the inside out makes it flatten with time — and the old stars that should carry the steeper history have moved several kiloparsecs from where they were born.
Named alongside it
The objects these essays reach for when they reach for this one.
Abundance gradientAge metallicity relationAngular momentumAngular momentum transportChemical evolutionCorotationCorotation resonanceDensity waveDepletion timeDisc heatingEpicyclic frequencyGalactic outflow