SIMBAD references

We note that nearby galaxies having high negative peculiar velocities are distributed over the sky very inhomogeneously. A part of this anisotropy is caused by the "Local Velocity Anomaly," i.e., by the bulk motion of nearby galaxies away from the Local Void. However, half of the fast-flying objects reside within a small region [R.A. = 11^h.5-13^h.0, decl. = +20°-40°] known as the Coma I cloud. According to Makarov & Karachentsev, this complex contains 8 groups, 5 triplets, 10 pairs, and 83 single galaxies with a total mass of 4.7x10¹³ M_☉. We use 122 galaxies in the Coma I region with known distances and radial velocities V_LG< 3000 km/s to draw the Hubble relation for them. The Hubble diagram shows a Z-shaped effect of infall with an amplitude of +200 km/s on the nearby side and -700 km/s on the back side. This phenomenon can be understood as the galaxy infall toward a dark attractor with a mass of ∼2x10¹⁴ M _☉ situated at a distance of 15 Mpc from us. The existence of a large void between the Coma and Virgo clusters also probably affects the Hubble flow around the Coma I.