TU Lyncis / TU Lyn
Light curve of the EA/GS type eclipsing binary TU Lyncis / TU Lyn, from photometry of 156 images taken with the Open University COAST telescope between 2017 July 27 and 2022 October 22 through a V filter.
The light curve appears to be varying slightly around the maxima with a somewhat sinusoidal shape to the curve.
This star is in the catalogues as an EA/GS variable (GCVS, AAVSO VSX, accessed 2023 July 13), with a period of 38.9461 days. Plotting a phase diagram of these observations with that period generates the following phase diagram.
This star is in the catalogues as an EA/GS variable (GCVS, AAVSO VSX, accessed 2023 July 13), with a period of 38.9461 days. Plotting a phase diagram of these observations with that period generates the following phase diagram.
An enlargement of the primary minimum appears below.
[This page updated 2023 July 13]