Morphology-dependent M_bh-σ0 relations are reported: shallow (2.5-3.1) for dust-poor S0 galaxies and steep (7.8) for massive ellipticals, using new SCOPE Bayesian regression on 137 galaxies.
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New SBF distance data confirm a steradian-scale flow converging at ~70 Mpc that matches the direction and amplitude of the CMB dipole and the original Great Attractor model.
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Return to the Great Attractor: Strong Evidence for a Steradian-sized Flow Converging at $\sim$70 Mpc within the GA Supercluster and Aligned with the CMB Dipole
New SBF distance data confirm a steradian-scale flow converging at ~70 Mpc that matches the direction and amplitude of the CMB dipole and the original Great Attractor model.