论文标题
M35，M67和M71银河系中的近二元星的光度研究
Photometric study of close binary stars in the M35, M67, and M71 Galactic clusters
论文作者
论文摘要
我们在年轻的开放群集M35，太阳能开放群集M67和球状群集M71中获得了近二元星的新多色光度法。使用100厘米（T100）望远镜在Tübítak国家天文台（TUG）进行了新的观察结果。我们提出了在选定的银河系簇中黯然失色的二进制系统的观察结果。获得了2个MASS J19532554 + 1851175、2MASS J19533427 + 1844047、2Mass J06092044 + 2415155和AH CNC的新的精确光曲线。分析了光曲线，我们得出了系统的一些轨道参数。
We obtained new multicolour photometry of close binary stars in the young open cluster M35, the solar-age open cluster M67, and the globular cluster M71. New observations have been carried out at the TÜBİTAK National Observatory (TUG) by using the 100cm (T100) telescope. We present observational results for eclipsing binary systems in the selected Galactic clusters. New accurate light curves for 2MASS J19532554 + 1851175, 2MASS J19533427 + 1844047, 2MASS J06092044 + 2415155, and AH Cnc were obtained. The light curves were analysed and we derived some of the orbital parameters of the systems.
