Flyby-induced high-eccentricity migration and the prevalence of hot Jupiters in M67

arXiv:2608.24874 · astro-ph.EP, astro-ph.GA, astro-ph.SR · Submitted 2026-08-25 · Read on arXiv

astro-ph.EP, astro-ph.GA, astro-ph.SR

Submitted: 2026-08-25

Updated: 2026-08-25

Comments: 25 pages, 13 figures, accepted for publication in MNRAS

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

Terminology

Hot Jupiter — 71× in this paper
Core — 30× in this paper · explained in 2 episodes
Tidal Disruption — 19× in this paper
Cold Jupiter — 10× in this paper
Mass Segregation — 10× in this paper · explained in 2 episodes
Consistency — 8× in this paper · explained in 3 episodes
Self-consistency — 6× in this paper · explained in 2 episodes
Velocity Dispersion — 5× in this paper · explained in 2 episodes
Population Synthesis — 4× in this paper · explained in 2 episodes
Adam — 3× in this paper · explained in 2 episodes
Hot Jupiter Candidate — 3× in this paper
Hybrid Approach — 3× in this paper · explained in 4 episodes
Metallicity — 3× in this paper · explained in 3 episodes
Secular Approximation — 3× in this paper · explained in 2 episodes
Dynamical regimes — 2× in this paper · explained in 2 episodes
Selection Bias — 2× in this paper · explained in 4 episodes
Trace — 2× in this paper · explained in 2 episodes
Warm Jupiter — 2× in this paper
Accuracy — 1× in this paper · explained in 1 episode
Benchmark — 1× in this paper · explained in 2 episodes
Momentum transfer — 1× in this paper · explained in 2 episodes
Robustness — 1× in this paper · explained in 5 episodes
Verification — 1× in this paper · explained in 2 episodes

Sources

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