长周期变星
- 网络Long-period variable
长周期变星-
渐近巨星分支（AGB）长周期变星研究进展
Progresses in Studies on AGB Long-period Variable Stars
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中等质量富金属AGB长周期变星的振动研究
Pulsations of Intermediate-Mass Metal-Rich AGB Long Period Variables
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按我们的观测，变星V879Sco不是一颗类似Tori的星云变星，而是长周期变星。
According to our observation the variable star V 879 Sco is a long period variable star .
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所选127个OH/IR脉泽源全部是有光学或红外证认的，其中大部分是光谱型>M5的长周期变星（主要是Mira变星）。
AM the selected OH / IR sources have optical or infrared identification . Most of them are associated with late-type ( > M5 ) Mira variables .
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V879Sco是一颗长周期变星
V 879 SCO is a long period variable star
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长周期变星的演化及振动
Evolution and Pulsation of Long Period Variables