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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 6.

Distribution of the number of ΔVs between any two components in the triples. The three velocities, ordered from lowest to highest, are labeled as V1, V2, and V3. The upper panel shows the ΔV distribution between any two components of the triple-star sample from Section 3, while the lower panel shows the same for the 132 triple-star candidates from C. Li et al. (2021). The black dashed line denotes ΔV between V2 − V1V2−1), the red dashed–dotted line shows ΔV between V3 − V2V3−2), and the blue solid line indicates ΔV between V3 − V1V3−1).

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