How to quench a galaxy
How central and satellite galaxies transition from star forming to quiescent
How central and satellite galaxies transition from star forming to quiescent
Gas before forming a disk galaxy: To be cool, or to be hot, that is the question.
Dr. Dara Norman shifts from magnification bias to representation bias in community tools such as white papers and advisory committees. Come learn about how access can fuel a revolution in inclusion at Dr. Norman’s talk at #AAS236.
In which cosmologists come up with yet another way to ignore pesky systematics – aka astrophysics!
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.
Tide goes in, dark matter halos come out, today’s authors can simulate that! With separate universe simulations!