An Open Cluster Origin for Most Solar-Type Binaries in the Solar Neighborhood and Implications for Primordial Planet Stability

arXiv:2609.22516 · astro-ph.SR, astro-ph.EP, astro-ph.GA · Submitted 2026-09-18 · Read on arXiv

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

Submitted: 2026-09-18

Updated: 2026-09-18

Comments: 7 pages, 3 figures, accepted for publication in ApJL

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

Terminology

• N-body simulations — 1× in this paper · explained in 2 episodes

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