EVOLUTION OF THE STARS
EVOLUTION OF THE STARS
复制标题
恒星的演化
DOI：
10.1143/ptps.22.1
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发表时间：
1963
影响因子：
--
通讯作者：
D. Sugimoto
中科院分区：
文献类型：
--
作者：
C. Hayashi;R. Hōshi;D. Sugimoto
将现代恒星演化理论尽可能扩展到氦燃烧、碳燃烧和后期燃烧阶段，并将理论结果与星团的Hertzsprung-Russell图进行了比较。讨论的主题包括中微子的核产生和能量损失，准静态平衡，包层，核心和表面溶液，化学成分均匀的恒星模型，氢燃烧阶段，氦燃烧阶段，核燃烧的高级阶段，朝向白矮星的初始阶段，以及主序列收缩阶段。(C.E.S.)
Modern theories on the evolution of stars are extended to the phases of helium burning, carbon burning, and later burnings as far as possible, and the theoretical results are compared wth the Hertzsprung-Russell diagrams of star clusters. The topics discussed include nuclear generation and energy loss by neutrinos, quasi-static equilibrium, envelope,core, and surface solutions, stellar models with homogeneous chemical composition, hydrogen burning phase, helium burning phase, advanced phases of nuclear burning, iinal phase toward white dwarfs, and pre-mainsequence contricting phase. (C.E.S.)