  Using archival HST/WFPC2 imaging of 7 LMC globular clusters, and following
the methods outlined in our previous study, we have reached the tightest
constrain so far on their age dispersion, which cannot be greater than ~ 0.5
Gyr. We also confirm earlier results that their average age is comparable to
that of the metal-poor Galactic globulars. Evidence is also provided that NGC
1841 is younger than the rest of LMC globulars.
