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Identifying Signatures of Inflow onto Face-on Galaxies Using the Balmer Decrement

Authors: Meghna Sitaram, Hui Li, Yong Zheng, Greg L. Bryan, Mary Putman, Aaron Smith, Rahul Kannan

Meghna Sitaram et al 2026 The Astrophysical Journal 1001 .

Provider: AAS Journals

Caption: Figure 4.

All panels show colormaps of the mass flux of gas at temperatures between 3 × 10³ and 5 × 10⁴ K across a slice of the galaxy with slice height labeled on the bottom right. Green corresponds to inflow, and pink corresponds to outflow. Gray regions show pixels where there are no warm gas particles.

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