Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death

@article{Groh2013FundamentalPO,
  title={Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death},
  author={J. Groh and G. Meynet and C. Georgy and S. Ekstrom},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={558}
}
We investigate the fundamental properties of core-collapse Supernova (SN) progenitors from single stars at solar meta llicity. For this purpose, we combine Geneva stellar evolutionary models with initial masses of Mini = 20− 120 M⊙ with atmospheric/wind models using the radiative transfer code CMFGEN. We provide synthetic photometry and high-resolution spectra of hot stars at t he pre-SN stage. For models with Mini = 9− 20 M⊙, we supplement our analysis using publicly available MARCS model… Expand
Predicting the nature of supernova progenitors
  • J. Groh
  • Physics, Medicine
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
  • 2017
Observational Constraints on the Progenitors of Core-Collapse Supernovae: The Case for Missing High-Mass Stars
  • S. Smartt
  • Physics
  • Publications of the Astronomical Society of Australia
  • 2015
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