I explore the intricate relationship between the interstellar medium, star formation, and feedback and its role in how galaxies evolve.
My research links the properties of the interstellar medium (ISM) from large scales measured in extragalactic sources to the small scales observed within the Milky Way. Linking large and small ISM scales offers insight into many key open questions about the role of the ISM and star formation in galaxy evolution, including: How is interstellar turbulence driven? How do molecular clouds form? What role does the atomic ISM play in the evolution of molecular clouds?
Check my Github profile for a full list of projects.
Looking for beautiful 21-cm HI maps of the Local Group galaxies? Look no further!
8 arcsec HI VLA maps of M33
A complete HI VLA mosaic of M31 at 58 arcsec
10 and 18 arcsec HI VLA mosaics of the northern half of M31 (overlaps with PHAT)
Data hosted by the Canadian Advanced Network for Astronomical Research (CANFAR).