Assistant Research Scientist at Johns Hopkins University
Research
I am an assistant research scientist at Johns Hopkins University working with Molly Peeples, Jason Tumlinson, and the rest of the fantastic FOGGIE team. I use cosmological simulations to study galaxies that are difficult to study with telescopes: the small, the dim, and the diffuse. I am a member of The N-Body Shop Collaboration, and many of the simulations that I use are run with N-body+SPH code Gasoline or its newer cousin, ChaNGa. However, I have also recently begun working with the FOGGIE simulations, which are run with Enzo.
Dwarf Galaxies
Stream of gas from merging galaxies (lower right) strikes dwarf galaxy (center; virial radius indicated by white circle), causing
neutral hydrogen (HI) to build up and eventually reigniting star formation. Click for larger version of gif.
I investigate dwarf galaxies that are initially quenched by reionization, but which resume star formation at least 2 Gyr later. In zoom-in simulations run with Gasoline,
star formation is restarted in these galaxies when they are struck by a stream of gas, typically either thrown off during a nearby merger (as in the
above gif) or simply hanging off of a neighboring galaxy. If the ram pressure exerted by the stream is within the right range, some of the gas in the halo of the dwarf is compressed onto its disk, forming neutral hydrogen (HI) and, eventually, stars. I am interested in how the gas within dwarf
galaxies evolves and, in particular, the role that environment plays in shaping their gas accretion and star formation histories.
Ultra-Diffuse Galaxies
Formation of a field ultra-diffuse galaxy in the Romulus25 cosmological simulation. An early merger causes star formation in the galaxy to relocate to its outskirts, reducing its central surface brightness and increasing its size. Click for a full version of the movie with gas.
Ultra-diffuse galaxies (UDGs) are galaxies that are both exceptionally large (reff > 1.5 kpc) and exceptionally low surface brightness (μ 0 > 24 mag/arcsec2). Although
originally discovered in clusters, they have also been observed in the field,
which suggests that it is not purely the violence of the cluster environment that creates them. However, it turns out that a galaxy that is isolated now didn't necessarily spend its entire life alone. The field UDGs that form within the Romulus25 cosmological simulation are primarily the products of relatively early major mergers that caused their star formation to move outward. I am interested in the properties and origins of these galaxies and other members of the low surface brightness galaxy family.
Demonstrating how smoke rings are made for a class of second graders in Newark
I received my B.S. in Astrophysics from Rice University in 2014 and my Ph.D. in Physics & Astronomy from Rutgers University in 2020. While at Rutgers, I served on the Graduate Student Organization (GSO)
and the Graduate Student Life Committee, helped to organize visits for prospective students, and participated in K-12 outreach. In my spare time,
I enjoy reading, baking, going for walks, and the occasional bit of recreational coding.
Due to the pandemic, I don't currently have an office, but feel free to send me an email at acwright*at*jhu.edu!
