Abstract
We present a new photoelectric light curve of α Coronae Borealis. The derived rate of apsidal motion differs from the theoretical prediction. A possible solution of the problem is suggested.
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Volkov, I.M. (2005). The Unique Binary Star α Coronae Borealis. In: Drechsel, H., Zejda, M. (eds) Zdeněk Kopal’s Binary Star Legacy. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3875-5_10
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DOI: https://doi.org/10.1007/1-4020-3875-5_10
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Publisher Name: Springer, Dordrecht
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Online ISBN: 978-1-4020-3875-4
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