The Low-Mass Stars in Starburst Clusters
  If star formation depends strongly on the global properties of the environment in which they form, the slope of the IMF as well as the upper and lower mass cut-offs would be expected to vary significantly between violent starbursts and more quiescent star forming regions. To test this hypothesis we observed the stellar content of the two closest massive star forming regions, 30Doradus and NGC3603 with HST/NICMOS and VLT/ISAAC. Our observations are the most sensitive observations made to date of dense starburst cores, allowing us to investigate its low-mass stellar population with unprecedented quality. The NIR luminosity function of 30Doradus shows no evidence for a truncation down to at least 1 M_o, its stellar core R136 is populated in low-mass stars to at least 2 M_o and NGC3603, which is very similar to R136, down to 0.1 M_o. Our observations clearly show that low-mass stars do form in massive starbursts. 
Bernhard Brandl (1), the NGC3603 and the 30Doradus-Team ((1) Cornell   University)