  We present lunar occultation observations obtained in August 2006 with the
recently demonstrated burst mode of the ISAAC instrument at the ESO VLT. The
results presented here follow the previously reported observations carried out
in March 2006 on a similar but unrelated set of sources.
  Interstellar extinction in the inner regions of the galactic bulge amounts to
tens of magnitudes at visual wavelengths. As a consequence, the majority of
sources in that area are poorly studied and large numbers of potentially
interesting sources such as late-type giants with circumstellar shells, stellar
masers, infrared stars, remain excluded from the typical investigations which
are carried out in less problematic regions. Also undetected are a large
numbers of binaries. By observing LO events in this region, we gain the means
to investigate at least a selected number of sources with an unprecedented
combination of sensitivity and angular resolution. The LO technique permits to
achieve mas resolution with a sensitivity of K~12mag at a very large telescope.
We have used the opportunity of a favorable passage of the Moon over a crowded
region in the general direction of the Galactic Center to observe 78 LO events
of heavily reddened stellar sources. We have detected six new binary and one
triple star, with typical projected separation of ~0.01". We have also detected
the compact circumstellar emission around one maser and one central star of a
planetary nebula. Additionally we have measured the diameter and/or
circumstellar shell of two carbon stars and other IR sources. In agreement with
our previous result, we conclude that lunar occultations in fast read-out mode
on a detector subwindow at an 8m-class telescope can achieve an angular
resolution close to 0.001" with a sensitivity K~12mag.
