On the Core-Collapse Supernova Explanation for LAMOST J1010+2358

S K Jeena, Projjwal Banerjee, Alexander Heger

Low-metallicity very massive stars with an initial mass of $\sim 140$--$260{\mathrm{M}}_{\odot }$ are expected to end their lives as pair-instability supernovae (PISNe). The abundance p…