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Secular bar formation in galaxies with significant amount of dark matter

Monthly Notices of the Royal Astronomical Society, no. 2 (2003): 406-422

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Using high-resolution N-body simulations of stellar discs embedded in cosmologically motivated dark matter haloes, we study the evolution of bars and the transfer of angular momentum between haloes and bars. We find that dynamical friction results in some transfer of angular momentum to the halo, but the effect is much smaller than previo...更多

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