  We used resolved star counts from Hubble Space Telescope images to determine
the center of gravity and the projected density profiles of 6 old globular
clusters in the Large Magellanic Cloud (LMC), namely NGC 1466, NGC 1841, NGC
1898, NGC 2210, NGC 2257 and Hodge 11. For each system, the LMC field
contribution was properly taken into account by making use, when needed, of
parallel HST observations. The derived values of the center of gravity may
differ by several arcseconds (corresponding to more than 1 pc at the distance
of the LMC) from previous determinations. The cluster density profiles are all
well fit by King models, with structural parameters that may differ from the
literature ones by even factors of two. Similarly to what observed for Galactic
globular clusters, the ratio between the effective and the core radii has been
found to anti-correlate with the cluster dynamical age.
