Abstract (EN):
We discuss the new results on the effects of convective overshooting in the PMS evolution of intermediate mass stars. These effects are extremely important in the end of the PMS, when the abundances in CNO elements approach the equilibrium in the centre. A moderate amount of overshooting produces, as the star approaches the ZAMS, an extra loop in the evolutionary tracks on the HR diagram; the amount of overshooting needed to produce the loop decreases with the stellar mass. An interesting feature is that there is a very well defined amount of overshooting (for a given stellar mass and chemical composition) beyond which a loop is produced; for smaller amounts of overshooting such a loop does not take place and the evolutionary tracks are similar to the ones obtained by Then (1965). We discuss the reasons for this behaviour and argue that it can provide a crucial observational test for convective overshooting in the core of intermediate mass stars.
Language:
English
Type (Professor's evaluation):
Scientific
No. of pages:
4