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Identifying Active Young Stars from the LAMOST MRS and TESS Survey

  • Authors: Fu-Kun Xu, Shenghong Gu, Yue Xiang

Fu-Kun Xu et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 6.

The youthfulness and activity of the ROT candidates. Left: distribution of lithium absorption strength as a function of rotation period. The data are color coded by Teff, and the lines show the binned median trends for Teff groups. Right: the Hα emission strength versus the Rossby number. The vertical lines indicate the transition among activity saturation regimes (see Figure 4, upper-right panel).

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