Massive stars live fast and die young, making metals along the way.
Meet Leo I, one of the dwarf galaxies that may help us understand the earliest galaxies to form.
Violent collisions give rise to some of the densest, most massive planets in our galaxy.
What’s even faster and more furious than Vin Diesel? Come learn about galactic winds at Dr. Christy Tremonti’s talk at #AAS236!
Is there a M∗-SFR-Z relation at high redshift? Yep! Read me to find how it was discovered!
A lot of physics happens below the resolution limit of galaxy simulations that must be represented with “subgrid” models. Today’s paper shows the importance of including a subgrid model for the mixing of metals in galaxy simulations.