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Identifying Hierarchically Triple Star Systems with Gaia DR3 and LAMOST

  • Authors: Tongyu He, Jiao Li, Jiangdan Li, Jianping Xiong, Xiaobin Zhang, Mikhail Kovalev, Qiyuan Cheng, Sufen Guo, Mingkuan Yang, Xuefei Chen, Zhanwen Han

Tongyu He et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 9.

MCMC corner plot for the triple-star system Gaia DR3 249662295687401216. The fitted model parameters are: for the inner binary: q1 = 0.919 ± 0.006, ﹩{K}_{1}=138.79{8}_{-0.749}^{+0.727}﹩, ﹩\sqrt{{e}_{1}}\cos {\omega }_{1}=0﹩, ﹩\sqrt{{e}_{1}}\sin {\omega }_{1}=0.0014\pm 0.001﹩; outer binary: ﹩\sqrt{{e}_{2}}\cos {\omega }_{2}=-0.00{8}_{-0.008}^{+0.015}﹩, ﹩\sqrt{{e}_{2}}\sin {\omega }_{2}=0.14{4}_{-0.068}^{+0.085}﹩, ﹩{q}_{2}=\mathrm{0.0.42}{7}_{-0.068}^{+0.077}﹩, ﹩{K}_{3}=21.27{5}_{-1.484}^{+1.752}﹩; and the system velocity: ﹩\gamma =7.7{4}_{-0.988}^{+1.038}\,\,{\rm{km s}}^{-1}\,﹩.

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