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Henize 2-10 (He 2-10) is a nearby (D = 9 Mpc) starbursting blue compact dwarfgalaxy that boasts a high star formation rate and a low luminosity AGN. He 2-10is also one of the first galaxies in which embedded superstar clusters (SSCs)were discovered. SSCs are massive, compact star clusters that will impact theirhost galaxies dramatically when their massive stars evolve. Here, we discussradio, submillimeter, and infrared observations of He 2-10 from 1.87 microns to6 cm in high angular resolution (~0.3 arcsec), which allows us to disentangleindividual clusters from aggregate complexes as identified at lower resolution.These results indicate the importance of spatial resolution to characterizeSSCs, as low resolution studies of SSCs average over aggregate complexes thatmay host SSCs at different stages of evolution. We explore the thermal,non-thermal, and dust emission associated with the clusters along with densemolecular tracers to construct a holistic review of the natal SSCs that haveyet to dramatically disrupt their parent molecular clouds. We assess theproduction rate of ionizing photons, extinction, total mass, and the starformation efficiency associated with the clusters. Notably, we find that thestar formation efficiency for the some of the natal clusters is high (>70%),which suggests that these clusters could remain bound even after the gas isdispersed from the system from stellar feedback mechanisms. If they remainbound, these SSCs could survive to become objects indistinguishable fromglobular clusters.

Towards a More Complex Understanding of Natal Super Star Clusters with Multiwavelength Observations