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• W2090900719 abstract "We use a new redshift survey complete to mR≃15.4 within 425 from the center of the Coma cluster to measure the mass profile of the cluster to r~5.5 h-1 Mpc. We extend the profile to r~10 h-1 Mpc with a further sample complete to mR=15.4 in 42% of the area within a 10° radius and to m=15.5 in the remaining area. Galaxies within this region are falling onto the cluster on moderately radial orbits and thus do not satisfy virial equilibrium. Nonetheless, identification of the caustics in redshift space provides an estimate of the gravitational potential at radius r and hence of the system mass, M(≤10 h-1 Mpc)=(1.65±0.41)×1015 h-1 M (1 σ error). Previous mass estimates derived from optical and X-ray observations are limited to r≤2.5 h-1 Mpc. Our mass profile is consistent with these estimates but extends to distances 4 times as large. Over the entire range, the mass increases with r at the rate expected for a Navarro, Frenk, & White density profile." @default.
• W2090900719 created "2016-06-24" @default.
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• W2090900719 date "1999-05-20" @default.
• W2090900719 modified "2023-09-27" @default.
• W2090900719 title "The Mass Profile of the Coma Galaxy Cluster" @default.
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• W2090900719 doi "https://doi.org/10.1086/312024" @default.
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