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Paper detail

Discovery of a W UMa type binary GSC 03553-00845

When observing the transiting extrasolar planets, we discovered a new W UMa type binary GSC 03553-00845. Following observation was carried out using the 1m telescope at Weihai Observatory of Shandong University. Complete BVR light curves were determined. Using the W-D program, we analyzed the light curves. Photometric solution reveals that GSC 03553-00845 is a W-subtype W UMa type binary with a mass ratio of q=2.904, it is an overcontact binary system by a contact degree of f=29.5% with a small temperature difference between the components (ΔT=206 K indicating a good thermal contact between the components. More observation of GSC 03553-00845 is needed in order to analyze the light curve variation and orbital period change.

preprint2014arXivOpen access
D. -F. GuoK. LiS. -M. HuY. -G. JiangD. -Y. GaoX. Chen
astro-ph.SR
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D. -F. GuoK. LiS. -M. HuY. -G. JiangD. -Y. GaoX. Chen

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