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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 3.

Left: the mass flux of different slices of the galaxy at different z-positions above and below the disk. Four different snapshots of time are shown. Right: the same, but only for Hα-emitting gas between 3 × 103 K and 5 × 104 K. Regions of the plot corresponding to inflow and outflow are displayed in the right panel.

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