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The formation of massive stars is an outstanding problem in stellarevolution. However, it is expected that they are (predominantly) born inheirarchical environments within massive young clusters, which in turn arelocated within larger star forming complexes that reflect the underlyingstructure of the natal molecular cloud. Initial observations of such regionssuggest that multiple generations of stars and proto-stars are present,necessitating a multiwavelength approach to yield a full (proto-)stellarcensus; in this contribution we provide an overview of just such anobservational approach for Galactic examples, focusing on the G305 complex.

Multiple stellar generations in massive star forming complexes