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I review massive star formation in our Galaxy, focusing on initial conditionsin Infrared Dark Clouds (IRDCs), including the search for massive pre-stellarcores (PSCs), and modeling of later stages of massive protostars, i.e., hotmolecular cores (HMCs). I highlight how developments in astrochemistry, coupledwith rapidly improving theoretical/computational and observational capabilitiesare helping to improve our understanding of the complex process of massive starformation.

Fire from Ice - Massive Star Birth from Infrared Dark Clouds