STELLAR PULSATIONS ACROSS THE HR DIAGRAM: Part II
STELLAR PULSATIONS ACROSS THE HR DIAGRAM: Part II
复制标题
DOI：
10.1146/annurev.astro.34.1.551
复制
发表时间：
1995
影响因子：
33.3
通讯作者：
A. Gautschy;H. Saio
中科院分区：
文献类型：
--
作者：
A. Gautschy;H. Saio
在恒星演化的各个阶段，基本上整个质量域的恒星都可能变得脉动不稳定。它们将以变星的形式出现，其特征是……
▪ Abstract Stars over essentially the whole mass domain can become pulsationally unstable during various stages of their evolution. They will appear as variable stars with characteristics that are ...