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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 6.

Phase plots of T gas vs. the number density of the three C+ colliding partners for the t = 170 Myr snapshot (see also Figure 5). Here L CII is weighted with the abundance of each colliding partner. From left to right, each panel shows the number densities of atomic hydrogen (H I), molecular hydrogen (H2), and electrons (e). The black solid lines correspond to the critical density of each partner vs. T gas (Goldsmith et al. 2012). We find that collisional de-excitation is negligible.

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