Type Ib and IIb supernova progenitors in interacting binary systems

  title={Type Ib and IIb supernova progenitors in interacting binary systems},
  author={Sung-Chul Yoon and L. Dessart and A. Clocchiatti},
  journal={arXiv: Solar and Stellar Astrophysics},
We explore properties of Type Ib and IIb SN progenitors that are produced by stable mass transfer in binary systems, using a new grid of stellar evolution models from an initial primary mass in the range of 10 - 18 $\mathrm{M_\odot}$ at solar and Large Magellanic Cloud metallicities. We find that blue and yellow supergiant SN IIb progenitors (e.g., of SN 2008ax, SN 2011dh, SN 2016gkg) have a hydrogen envelope mass less than about 0.15 $\mathrm{M_\odot}$, mostly resulting from early Case B mass… Expand
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We investigate the evolution of Type Ib/c supernova (SN Ib/c) progenitors in close binary systems, using new evolutionary models that include the effects of rotation, with initial masses of 12-25 M ☉Expand
Evolutionary Models for Type Ib/c Supernova Progenitors
  • Sung-Chul Yoon
  • Physics
  • Publications of the Astronomical Society of Australia
  • 2015
Abstract SNe Ib/c mark the deaths of hydrogen-deficient massive stars. The evolutionary scenarios for SNe Ib/c progenitors involve many important physical processes including mass loss by winds andExpand
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