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The Origin of the [C II] Deficit in a Simulated Dwarf Galaxy Merger-driven Starburst

  • Authors: Thomas G. Bisbas, Stefanie Walch, Thorsten Naab, Natalia Lahén, Rodrigo Herrera-Camus, Ulrich P. Steinwandel, Constantina M. Fotopoulou, Chia-Yu Hu, Peter H. Johansson

Thomas G. Bisbas et al 2022 The Astrophysical Journal 934 .

  • Provider: AAS Journals

Caption: Figure 15.

Left panel: correlation of the theoretical ΛCII function (Equation (C11)) vs. n H. The ∝ n H and ﹩\propto {n}_{{\rm{H}}}^{2}﹩ relations are plotted for comparison. Right panel: theoretical vs. simulation C II cooling. The red solid line is the y = x function to guide the eye. As can be seen, the majority of the ΛCII function is well reproduced following the analytical expressions discussed in Appendix C.

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