Cool Stars 14 - Submitted Abstract # 99 This version created on 05 October 2006 Observations of Massive Young Clusters with the Great Observatories Scott Wolk, Harvard-Smithsonian Center for Astrophysics Tyler Bourke, Harvard-Smithsonian Center for Astrophysics Bradley Spitzbart, Harvard-Smithsonian Center for Astrophysics Elaine Winston, Harvard-Smithsonian Center for Astrophysics S. Thomas Megeath, University of Toledo The combination of spatial and spectral coverage allow us to use Chandra, Spitzer and HST to the study regions of massive star formation which have been inaccessible even from the ground until the last decade. We survey the state of our understanding by discussing data from 3 moderately massive star forming regions. In order of increasing distance and mass we start with NGC 1579, centered on the Be star LkHa101 We have used the X-ray data to demonstrate that the distance of the cluster is about 700 pc, in stark contrast to several recent distance estimates of less than 400 pc. The Spitzer data provide supporting evidence by demonstrating the cluster membership is inconsistent with the nearer distance. RCW 108 is a complex star forming region. The NIR and X-ray data indicate the existence of several distinct episodes of star formation continuing through the current epoch. The data supports the hypothesis that previously extant density enhancements within a cold cloud are pushed to collapse by the ram pressure from the winds of nearby young star. NGC 281 is a somewhat more massive and complex region. We have found evidence of high temperature plasma expanding away from the Eastern complex and triggering the active star formation in the molecular cloud to the west. ----------------------------------