Dry merger — where it appears
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
Two spins that cancel, and an orbit that leaves
Disc galaxies and ellipticals of the same stellar mass differ by a factor of five in how much angular momentum each gram of their stars carries. Adding spin vectors in random directions explains most of it — two mergers of equals, with the orbit's angular momentum handed to the dark halo, carry a disc down to where ellipticals sit — and whether a merger makes a spheroid or rebuilds a disc turns on one number the vectors do not supply.
A galaxy that grows faster by eating small
Two equal elliptical galaxies merge and the result has twice the mass and twice the size. A galaxy that takes in the same mass as thirty small companions ends up nearly four times the size. The difference is one line of the virial theorem, in which companions bring mass without much energy, and it may answer a puzzle thrown up by the first deep infrared surveys: the most massive galaxies at redshift two are a fifth of the size of anything like them today.
Named alongside it
The objects these essays reach for when they reach for this one.
Compact galaxyDynamical frictionElliptical galaxyFall relationFast and slow rotatorsGalaxy mergerGalaxy spinIntegral-field spectroscopyMorphologySize mass relationSpecific angular momentumTidal stripping