Unveiling the Galaxy: Dense Gas and Star Formation in the Milky Way

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This project aims to address one of the most fundamental problems in astrophysics - understanding how high-mass stars form - by utilising a new, innovative, purpose-designed astronomical survey. This project will generate new knowledge about the star formation process by interfacing theoretical predictions with novel observations, aided by the most accurate distances yet derived. Expected outcomes include a comprehensive understanding of star formation, and an unparalleled map of the dense gas structure of our Galaxy. This should provide significant benefits, such as the crucial insight needed to interpret future sensitive, high-resolution surveys with next generation, globe-spanning telescopes in which Australia is a key partner.