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Tracking Halo Orbits and Their Mass Evolution around Large-scale Filaments

  • Authors: Hannah Jhee, Hyunmi Song, Rory Smith, Jihye Shin, Inkyu Park, Clotilde Laigle

Hannah Jhee et al 2022 The Astrophysical Journal 940 .

  • Provider: AAS Journals

Caption: Figure 4.

Binned distribution of r 0 and ﹩{v}_{\max }﹩ of crossers color-coded by the current (z = 0) mass of halos (top) and time since formation t formed (bottom). For a given r 0, more massive halos tend to have lower ﹩{v}_{\max }﹩, and to form earlier.

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