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Investigating a self-consistent galactic potential with central mass
1993
Symposium - International astronomical union
Preserved Fulltext
The evolution of a barred galactic potential containing a central mass concentration is examined by means of a self-consistent 2-D N-body simulation. It is found that the bar weakens as the central mass grows and eventually dissolves, in agreement with earlier orbital studies of this problem.
doi:10.1017/s007418090012371x
fatcat:66p27jtfgbgy5a3bukp7lcu5ou