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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 6.

Temporal variations in bar strength A2 (upper panels) and CMC within the ﹩r=0.5\,\mathrm{kpc}﹩ regions (lower panels) for the cold- (left) and warm-disk models (right). In the cold-disk models, the bar strength increases rapidly and then decays after reaching a peak due to the increase in the CMC. In the warm-disk models, the bar and CMC grow more slowly and steadily. The bar strength at late time is anticorrelated with ﹩{f}_{\mathrm{gas}}﹩ in both cold- and warm-disk models.

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