Image Details
Caption: Figure 19.
Cosmicflows-1 peculiar radial velocities viewed in the SGY–SGZ plane, the third orthogonal viewing angle. Galaxies with measured distances are shown if located in the slice defined by −1500 km s −1 ⩽ SGX ⩽ 1500 km s −1. Radial peculiar velocity vectors in the CMB frame are again shown with blue for negative velocities and in red for positive velocities.
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