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Anchoring Stellar Age Indicators: A Cross Calibration of [C/N] and Gyrochronology Ages via the Age–Velocity Dispersion Relation

  • Authors: Yuxi(Lucy) Lu, Marc H. Pinsonneault, Yuan-Sen Ting, Phil R. Van-Lane, John D. Roberts, Jamie Tayar, Alexander Stone-Martinez, Amanda L. Ash

Yuxi(Lucy) Lu et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 11.

Left: recovery of the cluster samples obtained from the literature (T. Cantat-Gaudin et al. 2020; E. L. Hunt & S. Reffert 2023; L. Cavallo et al. 2024; P. R. Van-Lane et al. 2024). Middle: same as left but in logarithmic scale. Right: ages obtained from [C/N] compared to those from rotation periods using the relations calibrated in this work for the same clusters. After correcting for bias for [C/N] and gyrochronology as shown in Figure 10, we are able to achieve agreement between the cluster ages determined from both methods. However, more data are needed to perform better comparisons.

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