Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0

Understand

We present a new grid of presupernova models of massive stars extending in mass between 13 and 120 Msun, covering four metallicities (i.e.

• [Fe/H]=0, -1, -2 and -3) and three initial rotation velocities (i.e.
• 0, 150 and 300 km/s).
• The explosion has been simulated following three different assumptions in order to show how the yields depend on the remnant mass - initial mass relation.