The contact binary V344 Lacertae: Is it a triple system? Liu Liang1;2;3;4, Qian Shengbang1;2;3;4, Li Kai5, He Jiajia1;2;3, Li Linjia1;2;3, Zhao Ergang1;2;3 and Li Xuzhi1;2;3;4 Received ; accepted Not to appear in Nonlearned J., 45. 1Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu Dis- trict, Kunming, 650216, P. R. China (e-mail:
[email protected]) 2Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, P. R. China arXiv:2006.16475v1 [astro-ph.SR] 30 Jun 2020 3Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, P. R. China 4University of Chinese Academy of Sciences, Yuquan Road 19#, Sijingshang Block, 100049 Beijing, China 5Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Envi- ronment, Institute of Space Sciences, Shandong University, Weihai, 264209, China { 2 { ABSTRACT The V RI passbands light curves of V344 Lac were presented and analyzed by using the latest version of the W-D code. The observed spectrum reveals that V344 Lac is not an A3 type but would be a later F type star according to the yielded temperature. The results of solution show that V344 Lac is an A- subtype contact binary, with a mediate photometric mass ratio of 0:387 ± 0:003 and a mediate contact factor of 44:6 ± 3:0%. Based on the parallax given by Gaia, the parameters of the components are estimated as: M1 = 1:16 M , M2 = 0:45 M , R1 = 1:31 R , R2 = 0:88 R , L1 = 2:512 L , L2 = 1:057 L .