The Contribution of Starspots to the Lithium Spread in NGC 2264

@misc{luo2026contribution,
  title = {{The Contribution of Starspots to the Lithium Spread in NGC 2264}},
  author = {Yan Luo and Gregory J. Herczeg and Min Fang and Qinghui Sun and Xiaoting Fu},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.19653},
  eprint = {2609.19653},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.19653},
  note = {CC BY 4.0},
}

TY  - UNPB
TI  - The Contribution of Starspots to the Lithium Spread in NGC 2264
AU  - Yan Luo
AU  - Gregory J. Herczeg
AU  - Min Fang
AU  - Qinghui Sun
AU  - Xiaoting Fu
PY  - 2026
DA  - 2026/09/17
PB  - arXiv
DO  - 10.48550/arxiv.2609.19653
UR  - https://arxiv.org/abs/2609.19653
AB  - Star clusters with ages of a few Myr have a previously unexplained dispersion in the lithium equivalent widths. In this work, we show that much of the lithium spread of the young cluster NGC 2264 can be attributed to the observational presence of starspots. We demonstrate that the equivalent width of Li I 6708 Angstrom changes with observed spot coverage, using a sample of 15 Weak-Lined T Tauri Stars (WTTSs) with multi-epoch high-resolution ESPaDOnS spectra and photometry. To quantify the contribution of starspots, we construct an empirical two-component starspot model. When differences in visible spot coverage are taken into account, 68% of the WTTSs fall within the model-predicted EW(Li) dispersion for a range from 0-90% visible spot coverage. We find no correlation between the age spread or gravity and Li I equivalent width in NGC 2264. Our results suggest that invoking starspots can explain much of the apparent lithium spread in NGC 2264 and reduces but does not fully eliminate the need to invoke rotation-driven lithium depletion or other non-standard explanations at such young ages. Future simultaneous measurements of lithium and beryllium in young stars may provide an independent test of this scenario.
ER  -