Figure 4 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 4.

Snapshots of the logarithm of the stellar surface density ﹩{{\rm{\Sigma }}}_{s}﹩ for the warm-disk models at t = 0.8, 1.5, 2.0, and 3.0 Gyr from left to right. Each row corresponds to a model with ﹩{f}_{\mathrm{gas}}=0 \% ﹩, 5%, 7%, and 10% from top to bottom. The color bar labels ﹩{{\rm{\Sigma }}}_{s}/({M}_{\odot }\,{\mathrm{pc}}^{-2})﹩.

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