Fig. 7.
Coma cluster region in 2MRS data set. Left panel: galaxies in supergalactic longitude (SGL) and latitude (SGB) between heliocentric velocities 3500 and 10 500 km s−1. Middle and right panels: galaxies in supergalactic coordinates and heliocentric velocity plane. Red points show the central component of the Coma cluster detected using the Bayesian group finder. Blue points show another relatively large component (15 members) and green points show the galaxies in groups with three to four members. Grey points show all other galaxies in Coma cluster region.
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