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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 8.

Left panel: relation of the [C II]/FIR ratio vs. ΣFIR. Low [C II]/FIR ratios are tightly connected with high SFR values. Black circles are observations presented in Herrera-Camus et al. (2018). The solid line corresponds to the Muñoz & Oh (2016) relation (Equation (6)). Right panel: relation of the [C II]/FIR ratio vs. ΣSFR. Black crosses are spatially resolved observations of the KINGFISH program presented in Smith et al. (2017), and the solid line corresponds to their best-fit function (Equation (7)). In both panels, triangles represent our simulation data, which have been color-coded according to their SFR value.

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