Prof. Emily Strickland (WSU)

Recent observations of Milky Way-like systems produce intriguing satellite galaxy mass distributions where it appears there are large ranges of satellite galaxy masses not observed. However, these visible gaps are not present in theoretical models. 

I will present potential mass gap formation mechanisms, and describe how our results so far have added to our understanding of galaxy formation. I use high-resolution hydrodynamic (and corresponding dark matter only) simulations of Milky Way analog galaxies from the Feedback In Realistic Environments (FIRE) collaboration and observational data from the Satellites Around Galactic Analogs (SAGA) Survey to explore these satellite galaxy mass gaps. 

I will then pivot to a discussion of my teaching pedagogy, with a focus on improving student engagement and identifying gaps in student understanding. This will include examples, advice, and results from my time so far at Wayne State and beyond.