BVRI photometry of the eclipsing binary BS Vul
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We present a detailed study of the close eclipsing binary BS Vulpeculae. Although it is relatively bright (V: 10.9-11.6mag) and belongs to short-periodic variable stars...
本研究对密接食双星（close eclipsing binary）狐狸座BS（BS Vulpeculae）开展了详尽的分析。尽管该天体亮度相对可观（V波段视星等：10.9~11.6星等），且属于短周期变星……
