We propose to take near IR spectroscopy of a selected
 sample of sources from the Two Micron Galactic Survey
 (TMGS) catalogue which are located in the central inner
 bulge of the Milky Way. The aim of this proposal is
 to investigate what is the dominant stellar population
 in this region.

 By means of the TMGS catalogue we have selected a list
 of highly luminous near-IR objects, previously undetected,
 which are strong candidates to be situated in the inner
 bulge of the Galactic Centre, and whose spectral type
 and luminosity class determination form the primary
 objective of this proposal.