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- W2064933710 abstract "We use the radial velocity data for 414 galaxies in the Coma cluster region provided by Kent and Gunn and the results of applying a membership criterion to carry out a discussion on the dynamical aspects of the Coma cluster. Our analysis shows that the Coma cluster has no bulk rotation that is clearly a dynamical effect. Fitting with the King-Mitchie model we find a core radius of 5.2′ or 210 kpc at H0 = 50(km/s)/Mpc and a characteristic velocity dispersion of 935 km/s. Viewed dynamically, there is clear morphological segregation, and there is evidence that substructure exists in the central region." @default.
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- W2064933710 date "1994-04-01" @default.
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- W2064933710 title "Studies of Coma cluster of galaxies 5. Dynamical problems" @default.
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- W2064933710 doi "https://doi.org/10.1016/0275-1062(94)90098-1" @default.
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