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Comparison of the Core-Collapse Evolution of Two Nearly Equal Mass Progenitors
Stephen W. Bruenn, Andre Sieverding, Eric J. Lentz +6
We compare the core-collapse evolution of a pair of 15.8 stars with significantly different internal structures, a consequence of bimodal variability exhibited by massive…
The explosion of 929 stars as Type II supernovae : results from radiative-transfer modeling at one year after explosion
Luc Dessart, D. John Hillier, Tuguldur Sukhbold +2
We present a set of nonlocal thermodynamic equilibrium steady-state calculations of radiative transfer for one-year old type II supernovae (SNe) starting from state-of-the-art expl…
The Impact of Black Hole Formation on Population Averaged Supernova Yields
Emily J. Griffith, Tuguldur Sukhbold, David H. Weinberg +3
The landscape of black hole (BH) formation -- which massive stars explode as core-collapse supernovae (CCSN) and which implode to BHs -- profoundly affects the IMF-averaged nucleos…
Towards a Realistic Explosion Landscape for Binary Population Synthesis
Rachel A. Patton, Tuguldur Sukhbold
A crucial ingredient in population synthesis studies involving massive stars is the determination of whether they explode or implode in the end. While the final fate of a massive s…
Emission line models for the lowest-mass core collapse supernovae. I: Case study of a 9 one-dimensional neutrino-driven explosion
A. Jerkstrand, T. Ertl, H. -T. Janka +3
A large fraction of core-collapse supernovae (CCSNe), 30-50%, are expected to originate from the low-mass end of progenitors with . However, degeneracy…
Supernova Progenitors, Their Variability, and the Type IIP Supernova ASASSN-16fq in M66
C. S. Kochanek, M. Fraser, S. M. Adams +10
We identify a pre-explosion counterpart to the nearby Type IIP supernova ASASSN-16fq (SN 2016cok) in archival Hubble Space Telescope (HST) data. The source appears to be a blend of…