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Gamma Equulei
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Title: Staying star gamma Equ
Author: V.D. Bychkov, L.V. Bychkova, J. Madej, G.P. Topilskaya

We determined rotational period of practically nonrotating Ap star gamma Equ and claim Prot=97 years. This period is about 35000 times larger than the average rotational period among stars of the same spectral class. Paper discusses possible mechanism explaining the origin of this phenomenon.

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