RU Eri UBV differential light curves
收藏B2FIND2026-03-19 收录
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RU Eri is a near-contact eclipsing binary (V~9.24mag) with a 0.632-day orbital period. The Wilson-Devinney program is used to simultaneously solve new UBV light curves obtained...
RU Eri是一颗轨道周期为0.632天的近相接食双星，其V波段视星等约9.24等。本研究采用威尔逊-德维尼（Wilson-Devinney）程序，对新获取的UBV光变曲线进行同步求解
