Pair-instability supernovae (PISNe) have crucial implications for many astrophysical topics,
including the search for very massive stars, the black hole mass spectrum, and galaxy …

Context. Carbon, nitrogen, and oxygen are the most abundant elements throughout the
universe, after hydrogen and helium. Studying these elements in low-metallicity stars can …

Recent advancements in stellar evolution modeling offer unprecedented accuracy in
predicting the evolution and deaths of stars. We present new stellar evolutionary models …

We use the inertial-inflow model of massive star formation to describe the formation of
globular clusters (GCs) in turbulent molecular clouds. A key aspect of this model is that the …

The fate of massive stars depends largely on the mass and structure of their inner cores, and
the composition of their envelopes at death. This is dependent on the mass loss history of …