Image Details

Choose export citation format:

Modeling the Atomic-to-molecular Transition in Cosmological Simulations of Galaxy Formation

  • Authors: Benedikt Diemer, Adam R. H. Stevens, John C. Forbes, Federico Marinacci, Lars Hernquist, Claudia del P. Lagos, Amiel Sternberg, Annalisa Pillepich, Dylan Nelson, Gergö Popping, Francisco Villaescusa-Navarro, Paul Torrey, and Mark Vogelsberger

2018 The Astrophysical Journal Supplement Series 238 33.

  • Provider: AAS Journals

Caption: Figure 10.

Impact of the UV escape fraction on the ﹩{{\rm{H}}}_{2}﹩ mass fraction for the fiducial escape fraction of 10% (blue), an extremely low escape fraction (1%, brown), and no absorption (100%, pink). The lines show the predictions of the volumetric GK11 and K13 models, but the same figures for other H I/﹩{{\rm{H}}}_{2}﹩ models or the projection-based versions look almost identical. Given that the probed escape fractions (and thus overall UV strengths) vary by a factor of 100, the variation of the ﹩{{\rm{H}}}_{2}﹩ mass by a factor of about three is rather moderate.

Other Images in This Article

Show More

Copyright and Terms & Conditions