MAUNA: Multiphase Analysis of (U)LIRG Nuclear Activity
Tracing Gas, Fueling, and Feedback in Merging Galaxies
Galaxies are made of stars, gas, and black holes, and the interplay between these components determines how a galaxy grows over time. Stars and black holes can change the chemical content of the gas reservoir and/or eject it entirely from the galaxy through winds — an outcome particularly prevalent in interacting galaxy systems that can shut down future generations of star formation. MAUNA leverages new Keck and JWST integral-field spectroscopic observations to study the hot ionized and warm molecular gas phases in a representative sample of galaxy mergers, building a holistic picture of gas dynamics from the dusty nuclear cores out to the circumgalactic medium.
