My thesis work was in Professor Elena D'Onghia's group on interactions between dwarf galaxies. Much of her work focuses on dynamics of disks like our Milky Way. One of the issues is how spiral arms form, and you can play with an interactive version of her results here.
You can also check out our group's Github page to see publicly available code.
My thesis work focused on interactions between small galaxies. I use computation models to understand how these small systems grow, interact, and ultimately build larger systems like the Milky Way. In particular, I focus on Magellanic spirals - galaxies that, like the Large Magellanic Cloud, have misplaced bars, single spiral arms, or irregular features. I have written papers on how these galaxies interact, how they can contribute gas to our own galaxy in the form of cold gas streams, and how the satellite population may be different around them.
Some of my current work focuses on the interaction between the Large and Small Magellanic Clouds. My simulations explore how this interaction formed the complex and extensive stream of HI gas seen around the Clouds.
As part of my thesis project, I examined the role of interactions in causing the asymmetries in Magellanic Galaxies. We discovered that tidally induced asymmetric-disks can masquerade as offset bars in Magellanic Galaxies.
We use a custom version of the GalIC code to simulate isolated galaxies and evolve encounters with Gadget 3.
Understanding where stars are born is a fundamental problem for astrophysics. This project used detailed chemical data from the APOGEE survey of more than 100,000 stars in the Milky Way to determine if there were statistically significant groups of stars that may have been born together.
As a 2014 fellow at the International Summer Institute for Modeling in Astrophysics, I worked with Andreas Küpper on modeling the tidal stream of NGC 5466. Tidal streams act as unique probes of the dark matter halo of their environments. This work, along with new data from Jay Strader, will place strong contraints on the shape and total mass of the Milky Way. We use a Markov chain Monte Carlo to probe parameter space, where the likelihood function is drawn in real time from very efficient restricted N-Body simulations of the globular cluster in our test potential.
The Lyman Alpha Reference Sample (LARS) is a large Hubble project and international collaboration testing the escape of Lyman Alpha photons from distant galaxies.
LARS utilizes almost the entire electromagnetic spectrum: from UV and optical spectra that reveal intense star formation, to radio observations that probe the neutral hydrogen and molecular gas content. The survey started with 14 galaxies and 28 more have now been added through e(xtended)LARS. We have conducted HI observations using the GBT, VLA, and GMRT of all 14 LARS galaxies and many of the 28 eLARS.
In 2014, we released the results for the first 14 galaxies. A few years later we added to this by carrying out similar measurements on a strange galaxy (Haro 11) that emits lots of Lyman Alpha and Lyman Continuum emission.