Figure 10 from Effects of Gas on Formation and Evolution of Stellar Bars and Nuclear Rings in Disk Galaxies

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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 10.

Temporal changes of ﹩{ \mathcal R }\equiv {R}_{\mathrm{CR}}/{R}_{b}﹩ for bars formed in the warm (solid) and cold disks (dashed). The shaded regions correspond to ﹩1\leqslant { \mathcal R }\leqslant 1.4﹩. Except for a brief period in the formation stage, all bars in our models are slow rotators.

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