Testing an Ap-like Magnetic Braking Origin for the Extended Main Sequence in Young Open Clusters

arXiv:2607.04152 · astro-ph.SR · Submitted 2026-07-05 · Read on arXiv

Chengyuan Li

astro-ph.SR

Submitted: 2026-07-05

Comments: 13 pages, 4 figures, accepted by the Astrophysical Journal

Project page: https://www.cosmos.esa.int/gaia

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Calibration — 3× in this paper · explained in 7 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Abundance — 1× in this paper · explained in 1 episode
• European Space Agency — 1× in this paper
• Gaia Data Processing and Analysis Consortium — 1× in this paper
• Robustness — 1× in this paper · explained in 5 episodes
• Spectral Signature — 1× in this paper · explained in 2 episodes
• Verification — 1× in this paper · explained in 2 episodes

Sources

• Properties of a volume-limited sample of magnetic Ap/Bp stars

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