周期变星

IRAS14122－5947：一颗新发现的超长周期变星

IRAS 14122-5947 : A Newly Discovered Variable Star with Extra Long Period

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

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

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 .

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 .

V879Sco是一颗长周期变星

V 879 SCO is a long period variable star

长周期变星的演化及振动

Evolution and Pulsation of Long Period Variables

短周期激变变星周期分布的新统计

Newly Statistics on the Period Distribution of Short-Period CVs

热超短周期造父变星的共性

The general properties of hot ultrashort period Cepheids