Enigmatic Explosions: How Different Supernova Models Yield Very Different Galaxies
Accounting for the uncertainty in supernova explosion parameters can substantially change the star formation history and morphology of galaxy simulations.
The Missing Link: New Insights from Post-starburst Outflows
What can outflowing gas tell us about the connection between rapid galaxy growth and AGN activity?
How to Break Through a Wall in the Universe?
Mysterious emissions are coming from the other side of the wall in a quasar!
Make Our Galaxy Grow: Massive Disk Galaxies in the Local Universe
Major galaxy mergers are thought to be one of the main ways of producing massive elliptical galaxies. Surprisingly though, some of the most massive galaxies in the local universe have gas disks. Here’s how they might be made.
The Grand Twirl
How well a galaxy dances may be a matter of life or death.
The Times They Are A-Changin’ (But the Stellar Mass Function of Massive Galaxies is Not!)
Massive galaxies arise by the time the universe is less than half its current age. Wait four billion more years, and by how much do these galaxies grow? The answer may surprise you.