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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 1.

Comparison of the CCF peak values for Gaia DR3 2077667962475652864 using different template spectra. In the upper part of the figure shows the normalized spectra. In the lower part of the figure, we present the generated CCF, A1 = 0.53, V1 = −131 km s−1, A2 = 0.48, V2 = 134 km s−1, and A3 = 0.41, V3 = 19 km s−1. The black solid line represents a template spectrum with a temperature of 7862 K, while the gray dashed line represents a CCF generated using a conventional solar spectrum template.

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