Presupernova evolution of massive stars

Ken'ichi Nomoto, Masa aki Hashimoto

研究成果: ジャーナルへの寄稿記事

309 引用 (Scopus)

抜粋

New presupernova evolutionary models of massive stars are presented. Improvements compared with the previous models are the inclusion of Coulomb interaction in the equation of state, electron capture from the beginning of oxygen burning, and many links between the silicon and iron quasi-equilibrium clusters during silicon burning. The iron core is found to be significantly smaller than in the previous models, especially for stars smaller than 15 M.

元の言語英語
ページ(範囲)13-36
ページ数24
ジャーナルPhysics Reports
163
発行部数1-3
DOI
出版物ステータス出版済み - 6 1988

    フィンガープリント

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

これを引用