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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 17.

Effect of choosing different lower observational limit for L CII. Top left: time evolution of the observational surface for the four different L CII lower limits considered. Top right: the ΣSFR − ΣCII relation. Bottom left: the [C II]/FIR ratio vs. ΣFIR. Bottom right: the [C II]/FIR ratio vs. ΣSFR. In all panels, the blue color is for L CII > 0 L , orange for L CII > 0.1 L , green for L CII > 0.5 L (the one we consider in the main text), and red for L CII > 1 L . As can be seen, the observational limit does not affect the trends and the overall results presented.

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