The dynamical state of bars in cluster dwarf galaxies: the cases of NGC 4483 and NGC 4516
Dwarf barred galaxies are the perfect candidates for hosting slowly rotating bars. They are common in dense environments and have a relatively shallow potential well, making them prone to heating by interactions. When an interaction induces bar formation, the bar should rotate slowly. They reside in massive and centrally concentrated dark matter
Cuomo, Virginia et al.
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2024