Golriz, S.S.Blommaert, J A D LVanhollebeke, EGroenewegen, M. A. T.Habing, H.J.Kemper, FSchultheis, MTielens, A.G.G.M.Waters, L B F MWood, Peter RCami, J2015-12-130035-8711http://hdl.handle.net/1885/75491We have selected a homogeneous sample of asymptotic giant branch (AGB) stars in theGalactic bulge population from the ISOGAL survey. Our target stars cover a wide range of mass-loss rates (~10-8-10-4 M⊙ yr-1) and differ primarily by their age on the AGBAuthor/s retain copyright201410.1093/mnras/stu13172015-12-11