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- W2028873635 abstract "Schweizer F. has proposed that NGC 7252 (Arp 226) recently formed from the merger of two disk galaxies and will ultimately relax into an elliptical galaxy (1982, Ap. J., 252). The suspected collision event has been successfully simulated with a gravitational interaction code, thereby reinforcing the merger hypothesis for the origin of this object. A careful selection of the disk and orbital model parameters lead to a good match to the present appearance and dynamics of this galaxy. The best simulation relaxes into an object which morphologically and kinematically resembles a normal elliptical galaxy." @default.
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- W2028873635 date "1991-03-01" @default.
- W2028873635 modified "2023-10-18" @default.
- W2028873635 title "A merger scenario for NGC 7252 - A tale of two tails" @default.
- W2028873635 doi "https://doi.org/10.1086/169742" @default.
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