Not so Slow: Do Galactic Bars Slow Down?
Add to your list(s)
Download to your calendar using vCal
If you have a question about this talk, please contact Sandro Tacchella.
N-body simulations indicate that galactic bars should slow down over time, owing to the interaction between the bar and the dark matter halo. This stands in conflict with observations, which indicate quickly rotating bars. We show that in a simulation which includes the gas phase the bar does not slow down, and offer tentative explanations for the behavior.
This talk is part of the Galaxies Discussion Group series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
|