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- W1623872019 abstract "A set of N-body simulations of the merging of two identical spherical galaxies was performed using a special-purpose computer, GRAPE-1. It is found that the kinematic properties of the resulting merger remnants are consistent with those of observed elliptical galaxies. The ratios of the maximum rotation velocity to the velocity dispersion are smaller than 0.6, even in the case of large impact parameters" @default.
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- W1623872019 date "1991-12-01" @default.
- W1623872019 modified "2023-10-04" @default.
- W1623872019 title "Kinematic Structures of Merger Remnants" @default.
- W1623872019 hasPublicationYear "1991" @default.
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