Observations of the Most Massive Deeply Embedded Star Clusters in the Milky Way

We summarize our comprehensive gas surveys of some of the most luminous, deeply embedded (optically obscured) star formation regions in the Milky Way, which are the local cases of massive star clusters and/or associations in the making. Our approach emphasizes multi-scale, multi-resolution imaging in dust and free-free continuum, as well as in molecular- and hydrogen recombination lines, to trace the multiple gas components from 0.1 pc (core scale) all the way up to the scales of the entire giant molecular cloud (GMC), or $\sim 100$ pc. We highlight our results in W49A, the most luminous Galactic star formation region ($L\sim {10}^7{L}_{\odot }$), which appears to be forming a young massive cluster (or a binary star cluster) with $M_{\star }>5\times {10}^4{M}_{\odot }$ that may remain bound after gas dispersal. The surveyed sources share elements in common, in particular, the 10-100 pc scale GMCs are filamentary but have one or two central condensations (clumps) far denser than the surrounding filaments and that host the (forming) massive stars.