Classification algorithms based on neural network techniques and class
ical statistical methods are applied in order to study the circumstanc
es in which the bulge stars can be differentiated from other stars bel
onging to other Galactic components. The Galactic system is simulated
as a mixture of four components, thin disc, thick disc, halo and bulge
, according to certain stellar system models. Each component is define
d from specific distribution laws of mass, velocity, metallicity and a
ge.