Type II supernovae from 8-10 M asymptotic giant branch stars

Masaaki Hashimoto, Kohichi Iwamoto, Ken'ichi Nomoto

研究成果: Contribution to journalArticle査読

53 被引用数 (Scopus)

抄録

The final evolution of 8-10 M stars in the AGB phase is recalculated to clarify whether these stars undergo collapse or thermonuclear explosion. New electron capture rates based on the shell model wave functions are employed for the evolution of the degenerate O + Ne + Mg core. It is found that the difference between the old and new rates are too small to alter the earlier conclusion that the O + Ne + Mg core collapses. The optical appearance of the resultant supernova explosion of AGB stars are discussed for observational diagnostics. In particular, a possible connection of the AGB star model with SN 1993J is examined.

本文言語英語
ページ(範囲)L105-L108
ジャーナルAstrophysical Journal
414
2 PART 2
DOI
出版ステータス出版済み - 9 10 1993

All Science Journal Classification (ASJC) codes

  • 天文学と天体物理学
  • 宇宙惑星科学

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