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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 1.

H-R diagram of the initial sample. Left panel: the OC sample taken from E. L. Hunt & S. Reffert (2023). The red solid line corresponds to the fitted MS locus. Red dashed lines are shifted by ±0.5 mag relative to the fitted curve, while the pink dashed line is obtained by shifting the fitted curve upward by 2 mag. The shaded region is used to select the initial sample. Right panel: the WD-MS binary sample. Blue dots represent the MS components of WD-MS binaries. The red solid line corresponds to the fitted MS locus. Green dashed lines are shifted by ±1 mag relative to the fitted curve. The shaded region is used to select the initial sample.

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