S. Bisterzo

1 ta ish

University of Turin

1. The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>s</mml:mi></mml:math>process: Nuclear physics, stellar models, and observations

   F. Käppeler, R. Gallino, S. Bisterzo +1

   MaqolaOAOchiq kirish20112 iqtibos

   ABIABI:AkademIndex/2026.other.003877