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• W3100123407 abstract "Spiral structure in disk galaxies is modeled with nine collisionless N-body simulations including live disks, halos, and bulges with a range of masses. Two of these simulations make long-lasting and strong two-arm spiral wave modes that last for $sim5$ Gyr with constant pattern speed. These two had a light stellar disk and the largest values of the Toomre $Q$ parameter in the inner region at the time the spirals formed, suggesting the presence of a Q-barrier to wave propagation resulting from the bulge. The relative bulge mass in these cases is about 10%. Models with weak two-arm spirals had pattern speeds that followed the radial dependence of the Inner Lindblad Resonance." @default.
• W3100123407 created "2020-11-23" @default.
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• W3100123407 date "2016-07-25" @default.
• W3100123407 modified "2023-09-26" @default.
• W3100123407 title "LONG-LIVED SPIRAL STRUCTURE FOR GALAXIES WITH INTERMEDIATE-SIZE BULGES" @default.
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• W3100123407 doi "https://doi.org/10.3847/2041-8205/826/2/l21" @default.
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