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

  • Authors: Anna C. Childs, Aaron M. Geller

Anna C. Childs and Aaron M. Geller 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 2.

The synthetic OCs generated over 5 Gyr within 1 kpc with tdis,O and ﹩{t}_{{\rm{dis}},{\rm{sim}}}﹩ are shown in blue dots and green diamonds, respectively. We show the initial mass at age = 0 for all of the dissolved OCs over the last 5 Gyr, and we show the current mass and age of the surviving OCs. All recorded snapshots from our simulations are shown with orange dots.

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