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The Photometric Study of Neglected Short-Period Eclipsing Binary BS Vulpeculae
Published online by Cambridge University Press: 23 April 2012
Abstract
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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.
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- Copyright © International Astronomical Union 2012
References
Wilson, R. E. & Van Hamme, W., 2003, Computing Binary Stars Observables, the 4th edition of the W-D program., Ftp: astro.ufl.edu, directory pub/wilson/lcdc2003Google Scholar
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