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Our research focuses on star formation through leading global teams in infrared and radio surveys, including one project that will map nearly all young massive stars in the Milky Way. We conduct targeted follow-up observations using advanced velocity-resolved spectroscopy, infrared interferometry, and spectropolarimetry. By analyzing millimeter, submillimeter, and infrared molecular line emissions with chemical models, we explore dynamic processes. Additionally, we develop multidimensional, multifluid hydromagnetic models to understand the formation of Giant Molecular Clouds and their structural evolution.
Our work also examines diffuse astrophysical matter in diverse environments such as planet-forming discs, circumstellar discs around aging stars, stellar death outflows, starburst superwinds, and galaxy clusters hosting quasar-like active galactic nuclei.