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Future evolution of bound superclusters in an accelerating Universe

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Academic year: 2020

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Figure

Figure 1. Simulated mass distribution at a = 1 (left-hand column) and a = 100 (right-hand column)
Figure 2. Scatter plots of the mass of identified bound objects, M bound , against the mass of the virialized HOP halo that forms its core, M HOP
Figure 3. Evolution of one of the most massive objects in our simulation, with a present-day mass of M ∼ 6.8 × 10 15 h −1 M , at a = 1
Figure 4. Evolution of two different bound objects in the simulation. Each row shows the evolution of a single object at a = 1, a = 2, a = 5, a = 10 and a = 100
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