We are focusing on two galaxies to get a good idea of what is happening in their cores in order to understand AGN and galactic blowout. What is galactic blowout? That can best be explained with a picture. This picture was taken using Hubble Space Telescope by my advisor Gerald Cecil a while back. It is an image of central region of NGC 3079.

For that I have been learning how to use a hydrodynamics code called Athena. There were other codes I could have used (like VH-1 for example) but my other advisor Fabian Heitsch recommended Athena for this type of project. So I downloaded Athena and went to work figuring out how to use it. I would say that it is a very well written code (of the little that I have used it) and that it is very intuitive and easy to learn (it's written in C). Right now I have been making up some toy models to get a good sense of how it works and what I can do with it. Recently (this week) I have been working on getting the data out and into an interesting format (one that I can show people and wow them with). On that note I have a short video for you guys.
What I have here is an extremely simple (emphasis on extremely, and simple) model of the disk of a galaxy (a constant density disk with exponential fall off to halo densities, not very realistic but for now it works). I have insterted a "starburst" in the center with an over-pressure region (luminosity/supernova) along with some wind (i.e. kinetic energy, matter outflow). The computation is only doing 2D, and is small enough that I am running it on my laptop.
Here the x-y plane represents the computaion grid (250 grid points in the x, 500 in the y). The z axis is density. I took the output from Athena and fed it into MATLAB and turned it into a movie that I am posting here. I hope you enjoy. When I have real stuff (with good physical interpretation) I will post about that.