Image Details

Choose export citation format:

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 10.

Stacked phase-space trajectories (left) and mass evolution profiles (right) of halos in the five subsamples in Figure 9: 1/2 for recent crossers, 3/4 for intermediate crossers, 5 for ancient crossers, 1/3/5 for mass-gaining halos, and 2/4 for mass-losing halos. Because the first crossing moment differs between halos, individual mass evolution profiles are stacked after making the first crossing moment the zero-point (i.e., tt FC). That is, tt FC < 0 and > 0 are before and after the first crossing, respectively.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse