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- W205532270 abstract "We investigate by N-body simulations how a galaxy with an axisymmetric self-gravitating disc component responds to the tidal force of another galaxy. It is found that the inner region of the self-gravitating discs generally develop bar structures when perturbed by the tidal force. The results predict a higher incidence of barred systems in interacting galaxies and suggest that active nuclei in interacting galaxies are fuelled with the gas by tidally-induced bars." @default.
- W205532270 created "2016-06-24" @default.
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- W205532270 date "1988-01-01" @default.
- W205532270 modified "2023-10-02" @default.
- W205532270 title "Bar Formation in Interacting Galaxies" @default.
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- W205532270 doi "https://doi.org/10.1007/978-94-009-2917-3_61" @default.
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