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Evolution of Stellar Activity and Habitable Zone. IV. Calcium II Infrared Triplet Activity from Open Clusters and White Dwarf Binaries

  • Authors: Shidi Zhang, Song Wang, Henggeng Han, Wenyuan Cui

Shidi Zhang et al 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 4.

Comparison of log﹩{R}_{{\rm{IRT}},{\rm{base}}}^{{\prime} }﹩ and log﹩{R}_{{\rm{IRT}},{\rm{cat}}}^{{\prime} }﹩ measurements. Blue dots represent OC members, and red dots denote WD-MS binaries. The green line represents a linear fit to sources with log﹩{R}_{{\rm{IRT}},{\rm{cat}}}^{{\prime} }﹩ > −5.4. The black dashed line denotes a unity line. The gray dashed line is placed at log﹩{R}_{{\rm{IRT}},{\rm{cat}}}^{{\prime} }﹩ = −5.4, below which the ﹩{R}_{{\rm{IRT}},{\rm{cat}}}^{{\prime} }﹩ measurements may be unreliable (S. Freund et al. 2025).

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