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Figuring Out Gas and Galaxies in Enzo (FOGGIE). XIII. On the Observability of Extended H I Disks and Warps

  • Authors: Cameron W. Trapp, Molly S. Peeples, Jason Tumlinson, Brian W. O'Shea, Anna C. Wright, Ayan Acharyya, Britton D. Smith, Vida Saeedzadeh, Ramona Augustin

Cameron W. Trapp et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 4.

H I covering fraction (﹩{{ \mathcal L }}_{HI}﹩) as a function of impact parameter for the “smoothed” (solid) and “filtered” (dashed) moment-0 maps shown in Figures 2 and 3 at 20 Mpc. As expected, the curve for Maelstrom does not change significantly, as there is little diffuse material that is filtered out. For both Blizzard and Cyclone, the filtered curve is shifted to the left by a few kpc due to diffuse material being filtered out. Covering fractions are calculated in 2 kpc thick annuli centered on the given impact parameter.

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