NGTS clusters survey - VI: Stellar rotation in seven young open clusters within the PLATO LOPS2 field

arXiv:2608.27170 · astro-ph.SR, astro-ph.GA · Submitted 2026-08-27 · Read on arXiv

astro-ph.SR, astro-ph.GA

Submitted: 2026-08-27

Updated: 2026-08-27

Code: https://github.com/MNGuenther/tess_infos

Terminology

• Core — 22× in this paper · explained in 2 episodes
• Angular Momentum Loss — 3× in this paper · explained in 1 episode
• Benchmark — 3× in this paper · explained in 2 episodes
• Clustering — 3× in this paper · explained in 2 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Decoupling — 2× in this paper · explained in 2 episodes
• Mikulski Archive for Space Telescopes — 2× in this paper
• Science and Technology Facilities Council — 2× in this paper
• TESS All-Sky Rotation Survey — 2× in this paper
• Abundance — 1× in this paper · explained in 1 episode
• Accuracy — 1× in this paper · explained in 1 episode
• Aperture — 1× in this paper · explained in 1 episode
• Cluster Difference Imaging Photometric Survey — 1× in this paper
• European Space Agency — 1× in this paper
• Momentum transfer — 1× in this paper · explained in 2 episodes
• Quick Look Pipeline — 1× in this paper
• Sparsity — 1× in this paper · explained in 4 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• The TESS All-Sky Rotation Survey: Periods for 1,046,317 Stars Within 500 pc
• Evolution of binary stars and its implications for evolutionary population synthesis
• Accelerated Hierarchical Density Clustering
• The PLATO Mission

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