1) precataclysmic binary
激变前双星
2) precataclysmic variable
激变前变星
3) cataclysmic variable
激变变星
1.
Su UMa-type dwarf novas belong to cataclysmic variable stars, whose character is magnified explosion, i.
SUUMa -type矮新星属于激变变星 ,其特征是存在扩大了的爆发即超爆发。
2.
The photometrically and spectroscopically observational properties of cataclysmic variables have been reviewed.
评述了激变变星的测光,分光特
3.
It has been applied to the analyses of theshort period oscillations in ctalysmic variable V795 Her and pre-cataclysmic variableHW Vir.
并把它应用到激变变星V795Her和激变前变星HWVir的短周期振荡分析中，结果表明这两颗变星都有明显的闪变，在V795Her中还存在周期为265。
4) cataclysmic variables
激变变星
1.
In this paper, some CCD spectra of 6 cataclysmic variables: AB Boo, T CrB, UX UMa, AH Her, Z Cam, V426 Oph and 3 related objects: Leo3, UMa3 and EG UMa are presented.
16m望远镜卡焦光谱仪观测获得的6颗激变变星（ABBoo；UXUMa，TCrBAHHer，ZCam和V426Oph）及3颗相关天体（UMa3，EGUMa和Leo3）的CCD光谱，并同时拍摄了5颗晚型星（3Dra，Vir，Leo，34Boo和36Corn）的CCD光谱，作为晚型星参考谱。
5) magnetic cataclysmic variable
磁激变变星
6) binary flare star
耀变双星
补充资料：激变
急剧变化：形势～。
说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条