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.
The early universe is a period of intense star formation across nearly all galaxies. Is it possible tell these galaxies apart from each other, when the universe was less than a few billion years old?
Accounting for the uncertainty in supernova explosion parameters can substantially change the star formation history and morphology of galaxy simulations.
What can outflowing gas tell us about the connection between rapid galaxy growth and AGN activity?