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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 20.

Temporal variations in SFR and the gas mass in the ring regions at ﹩R\lt {R}_{\mathrm{ring}}+0.2\,\mathrm{kpc}﹩ (top), the bar regions at ﹩{R}_{\mathrm{ring}}+0.2\,\mathrm{kpc}\lt R\lt {R}_{b}+0.5\,\mathrm{kpc}﹩ (middle), and the arm regions at ﹩R\gt {R}_{b}+0.5\,\mathrm{kpc}﹩ (bottom). The left and right panels are for the cold- and warm-disk models, respectively.

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