Progenitors of Core-Collapse Supernovae

  title={Progenitors of Core-Collapse Supernovae},
  author={Steven J. Smartt},
  journal={Annual Review of Astronomy and Astrophysics},
  • S. Smartt
  • Published 5 August 2009
  • Physics
  • Annual Review of Astronomy and Astrophysics
Knowledge of the progenitors of core-collapse supernovae is a fundamental component in understanding the explosions. The recent progress in finding such stars is reviewed. The minimum initial mass that can produce a supernova (SN) has converged to 8 ± 1 M⊙ from direct detections of red supergiant progenitors of II-P SNe and the most massive white dwarf progenitors, although this value is model dependent. It appears that most type Ibc SNe arise from moderate mass interacting binaries. The highly… 
Progenitor constraints for core-collapse supernovae from Chandra X-ray observations
The progenitors of hydrogen-poor core-collapse supernovae (SNe) of types Ib, Ic and IIb are believed to have shed their outer hydrogen envelopes either by extremely strong stellar winds,
Predicting the nature of supernova progenitors
  • J. Groh
  • Physics
    Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
  • 2017
Recent efforts to predict the nature of stars before death by performing coupled stellar evolution and atmosphere modelling of single stars in the pre-SN stage are reviewed, and the detectability of SN Ibc progenitors is assessed.
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