Image Details

Choose export citation format:

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 1.

Scaling relations for the six H I disks presented in this study. The points correspond to the mean values for a given system between z = 0 and z = 0.5, with bars showing the standard deviation. Top: the H I size–mass relation (A. H. Broeils & M. H. Rhee 1997a) for these systems. MHI is calculated as the total disk H I mass. DHI is twice the radius at which the mean column density drops below 1.25 × 1020 cm−2. The solid (dashed) line corresponds to the observational correlation (and 3σ scatter) found in J. Wang et al. (2016).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse