YMC that encloses a total cluster mass in excess of 10$^5$$M_{\odot}$ within 10pc (Selman & Melnick 2013). The cluster contains roughly 200 massive stars ($>$8$M_{\odot}$) within a central region less than 6pc, whose radiation and mechanical feedback profoundly impact the surrounding medium (Schneider et al. 2017, subm.). R136 is the most massive YMC in our local neighbourhood that can be adequately resolved spatially (at 50kpc, the nominal distance to R136, 1$\arcsec$$\approx$0.25pc) enabling us observe individual objects at the star and molecular clump scale. This makes R136 an ideal laboratory to examine how feedback from massive stars affects further star formation (e.g. Dale et al. 2012).

The mechanical and radiation output from R136 has created a central cavity by sweeping the surrounding molecular clouds (labelled as clouds 6 and 10 in Fig.1) that extend up to 100pc along the northeast-southwest axis (Pellegrini et al. 2010). We adopt the cloud nomenclature of Johansson et al. (1998). Brightly illuminated arcs delineate the interfaces between the cold gas and the ionizing radiation, where subsequent generations of stars are thought to have been triggered (Walborn et al. 2002). Studies at optical (De Marchi et al. 2011; Kalari et al. 2014), near-infrared (nIR; Rubio et al. 