arXiv · 2505.18312
V965 Cephei revisited: evidence for a binary system
Abstract
We extended the $O-C$ diagram for V965 Cep with all currently available observations in the Johnson V filter and added unfiltered ones. The new, up-to-date $O-C$ diagram shows that the seeming period change previously revealed by the author does not occur uniformly. Instead, the near-parabolic part of the $O-C$ diagram can be a part of a periodic curve. This could be a sign of the second body in the system. Based on our observations, we also estimated the $B-V$ index of the star to be $0.48 \pm 0.05$ at maximum brightness and $0.57 \pm 0.05$ at minimum brightness.
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Maksym Pyatnytskyy. 2025-05-23. V965 Cephei revisited: evidence for a binary system. https://arxiv.org/abs/2505.18312
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