Advanced burning stages and fate of 8-10 M⊙ STARS

@article{Jones2013AdvancedBS,
  title={Advanced burning stages and fate of 8-10 M⊙ STARS},
  author={Samuel W. Jones and Raphael Hirschi and Ken’ichi Nomoto and Tobias Fischer and Francis X. Timmes and Falk Herwig and Bill Paxton and Hiroshi Toki and Toshio Suzuki and Gabriel Mart{\'i}nez-Pinedo and Y. H. Lam and Michael G. Bertolli Keele University and Kavli Ipmu and Gsi and Tu Darmstadt and Asu and Jin-a and Uvic and Kitp Ucsb and Osaka City University and Nihon University and Nao Japan and Lanl},
  journal={The Astrophysical Journal},
  year={2013},
  volume={772},
  pages={150}
}
The stellar mass range 8 {approx}< M/M{sub Sun} {approx}< 12 corresponds to the most massive asymptotic giant branch (AGB) stars and the most numerous massive stars. It is host to a variety of supernova (SN) progenitors and is therefore very important for galactic chemical evolution and stellar population studies. In this paper, we study the transition from super-AGB (SAGB) star to massive star and find that a propagating neon-oxygen-burning shell is common to both the most massive electron… 
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