Non standard s-process in massive rotating stars. Yields of $10-150$ $M_{\odot}$ models at $Z=10^{-3}$

Understand

Recent studies show that rotation significantly affects the s-process in massive stars.

• We provide tables of yields for non-rotating and rotating massive stars between 10 and 150 $M_{\odot}$ at $Z=10^{-3}$ ([Fe/H] $=-1.8$).
• Tables for different mass cuts are provided.
• The complete s-process is followed during the whole evolution with a network of 737 isotopes, from Hydrogen to Polonium.