  The expected microlensing events of the LMC by the MACHOs of the LMC itself
are calculated and compared with analogue events by objects in the Galactic
halo. The LMC matter distribution is modelled by a spherical halo and an
exponential disk while a face-on exponential disk is used for the stellar
distribution of the LMC. Among the microlensing events discovered by the MACHOs
and EROS projects, a fraction of $22\%$ could be caused by the lenses near the
center of the LMC or $13\%$ from lenses at $5^o$ from the LMC center.
Therefore, any statistical study of these microlensing events must take the LMC
lenses into account.
