# Type Ib and IIb supernova progenitors in interacting binary systems

@article{Yoon2017TypeIA,
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},
year={2017}
}
• Published 2017
• Physics
• 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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