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

@inproceedings{Jones2013AdvancedBS,
  title={Advanced burning stages and fate of 8-10 M⊙ STARS},
  author={Samuel Jones and Raphael Hirschi and Ken'ichi Nomoto and Tobias Fischer and Frank X. Timmes and Falk Herwig and B. D. Paxton and Hiroshi Toki and Toshio Suzuki and Gabriel Mart́ınez-Pinedo and Yi Hua Lam and Michael G. Bertolli Keele University and Kavli Ipmu and Gsi and Tu Darmstadt and Asu and Ji-na and UVic and Kitp Ucsb and Osaka University and Nihon University and Nao Japan and Lanl},
  year={2013}
}
  • Samuel Jones, Raphael Hirschi, +20 authors Lanl
  • Published 2013
  • Physics
  • The stellar mass range 8 M/M ? 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 capture supernova (EC-SN… CONTINUE READING

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