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Globular Clusters and Dark Satellite Galaxies through the Stream Velocity

  • Authors: Smadar Naoz and Ramesh Narayan

Naoz & Narayan 2014 The Astrophysical Journal Letters 791 L8.

  • Provider: AAS Journals

Caption: Figure 1.

Top panel: phase shift Δϕ between fluctuations in the baryons and DM as a function of redshift for modes with k = 200, 100, 40, 20 Mpc−1, assuming a stream velocity vbc = 1σvbc and θ = 0. Middle panel: comoving spatial separation between baryons and DM (solid lines) and comoving virial radius of the DM halo (dashed lines). Bottom panel: similar to the middle panel, but shows the physical spatial separation.

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