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Effects of Gas on Formation and Evolution of Stellar Bars and Nuclear Rings in Disk Galaxies

  • Authors: Woo-Young Seo, Woong-Tae Kim, SungWon Kwak, Pei-Ying Hsieh, Cheongho Han, and Phil F. Hopkins

2019 The Astrophysical Journal 872 5.

  • Provider: AAS Journals

Caption: Figure 21.

Sizes of nuclear rings against the dimensionless parameter ﹩{ \mathcal B }\propto \mathrm{CMC}/({A}_{2}^{0.3}{{\rm{\Omega }}}_{b}^{0.2})﹩ defined in Equation (12). The symbol sizes correspond to the simulation time. The dashed line draws ﹩{R}_{\mathrm{ring}}/(1\,\mathrm{kpc})=5{{ \mathcal B }}^{2}﹩, which fits the numerical results reasonably well, except for model C10 with the oval.

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