Fig. 1. The initial-final mass lelations. The solid line indicates our results of AGB evolution calculations based on the expressions from Iben and Truran (1978) and Renzini and Voli (1981), and assuming the coefficient in Reimers (1975) mass loss intensity law as for and for . The dashed line indicates the results of the calculations of Groenewegen and de Jong (1993). Dots represent the initial-final mass relations for stars in the Magellanic Cloud clusters (see text for details)