MESSINA, SergioSergioMESSINAHentunen, V. -P.V. -P.HentunenZambelli, R.R.Zambelli2020-04-162020-04-1620150374-0676http://hdl.handle.net/20.500.12386/24070We present the results of a multi-filter photometric monitoring of the wide binary HIP10680/HIP10679 WE found both component to be variable with amplitude up to delta V = 0.03 mag in the case of HIP10680 and delta V = 0.07 mag in the case of HIP10679. We could measure the rotation periods P = 0.2396 d of the hotter F5V component HIP10680 and P = 0.777 d of the cooler G5V component HIP10679. We found that the rotation axes of both components are aligned with an inclination i = 10.ELETTRONICOenArticlehttps://konkoly.hu/ibvs/6101.html2015IBVS.6145....1MFIS/05 - ASTRONOMIA E ASTROFISICA