Based on imaging and spectroscopy obtained at the ESO NTT telescope and usi
ng an efficient image analysis algorithm, we study the core of the LMC OB a
ssociation LH 13, particularly the two compact stellar clusters Sk-66 degre
es 41 and HNT in the H II region N 11C. We resolve Sk-66 degrees 41 into 15
components and for the first time the HNT cluster into 70 stars, and deriv
e photometry for the members. Moreover, from medium resolution spectroscopy
we determine the spectral types for sixteen stars in N 11C. We compare the
color-magnitude diagrams of the clusters with that of the field stars and
discuss the cluster ages. With an age of similar to 100 Myr, the HNT cluste
r appears significantly older than the very young (less than or equal to 5
Myr) Sk-66 degrees 41 starburst. We suggest that most of the 'field' O-star
s in the core of N 11C have actually been ejected from Sk-66 degrees 41 thr
ough dynamical interactions in the compact cluster. The properties of the S
k-66 degrees 41 and HNT clusters suggest that we are viewing different star
formation regions lying at different distances along the same line of sigh
t.