Towards a More Complex Understanding of Natal Super Star Clusters with
  Multiwavelength Observations
  Henize 2-10 (He 2-10) is a nearby (D = 9 Mpc) starbursting blue compact dwarf
galaxy that boasts a high star formation rate and a low luminosity AGN. He 2-10
is also one of the first galaxies in which embedded superstar clusters (SSCs)
were discovered. SSCs are massive, compact star clusters that will impact their
host galaxies dramatically when their massive stars evolve. Here, we discuss
radio, submillimeter, and infrared observations of He 2-10 from 1.87 microns to
6 cm in high angular resolution (~0.3 arcsec), which allows us to disentangle
individual clusters from aggregate complexes as identified at lower resolution.
These results indicate the importance of spatial resolution to characterize
SSCs, as low resolution studies of SSCs average over aggregate complexes that
may host SSCs at different stages of evolution. We explore the thermal,
non-thermal, and dust emission associated with the clusters along with dense
molecular tracers to construct a holistic review of the natal SSCs that have
yet to dramatically disrupt their parent molecular clouds. We assess the
production rate of ionizing photons, extinction, total mass, and the star
formation efficiency associated with the clusters. Notably, we find that the
star formation efficiency for the some of the natal clusters is high (>70%),
which suggests that these clusters could remain bound even after the gas is
dispersed from the system from stellar feedback mechanisms. If they remain
bound, these SSCs could survive to become objects indistinguishable from
globular clusters.
