The Photometric Study of Neglected Short-Period Eclipsing Binary BS Vulpeculae

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Authors	ZEJDA Miloslav MIKULÁŠEK Zdeněk ZHU Liying QIAN Shengbang LIŠKA Jiří
Year of publication	2012
Type	Article in Proceedings
Conference	FROM INTERACTING BINARIES TO EXOPLANETS: ESSENTIAL MODELING TOOLS
MU Faculty or unit	Faculty of Science
Citation
Doi	http://dx.doi.org/10.1017/S1743921311027001
Field	Astronomy and astrophysics
Keywords	stars: binaries: eclipsing; stars: fundamental parameters; stars: individual BS Vul
Description	The preliminary results of a study of a neglected, relatively bright, short-periodic (P=0.48 d), near contact eclipsing binary BS Vulpeculae is given. We present our new complete (BVRI) light curves, and physical parameters of the system based on them, derived by the 2003 version of the Wilson-Van Hamme code.
Related projects:	Mass-loss rate predictions for hot stars Spectral energy distribution of hot stars and its variability Fyzika hvězd a hvězdných soustav Photometric Investigation of Selected Eclipsing Binaries