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.
Sorting the Sombrero galaxy into a galaxy classification is difficult to do, but new evidence suggests that like Harry Potter, the Sombrero galaxy may fit into more than one category.
Hydrodynamical simulations shed new light on the metallicity of stellar populations in dwarf galaxies.