Galactic mass-losing AGB stars probed with the IRTS. II

We are using the 2002 data-release from the Japanese space experiment IRTS to investigate the spatial distribution of galactic masslosing ( (greater than) 2 10^-s M{dot} yr^-1) AGB stars and the relative contribution of C-rich and O-rich ones to the replenishment of the ISM. Our sample contains 126 C-rich and 563 O-rich sources which are sorted on the basis of the molecular bands observed in the range 1.4-4.0 (mu)m, and for which we estimate distances and mass loss rates from near-infrared photometry ( K and Lʹ). There is a clear dependence on galactocentric distance, with O-rich sources outnumbering C-rich ones for r{GC}(less than) 8 kpc, and the reverse for r {GC}(less than)10 kpc. The contribution to the replenishment of the ISM by O-rich AGB stars relative to C-rich ones follows the same trend. Although they are rare (~10% in our sample), sources with 10^-6 M{dot} yr^-1 (less than)M 10^-5 M{dot} yr^-1 dominate the replenishment of the ISM by contributing to ~50% of the total of the complete sample. We find 2 carbon stars at more than 1 kpc from the Galactic Plane, that probably belong to the halo of our Galaxy.