Figure 2 from ALMA [C I]3P1–3P0 Observations of NGC 6240: A Puzzling Molecular Outflow, and the Role of Outflows in the Global αCO Factor of (U)LIRGs

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ALMA [C I]³P₁–³P₀ Observations of NGC 6240: A Puzzling Molecular Outflow, and the Role of Outflows in the Global α_CO Factor of (U)LIRGs

Authors: Claudia Cicone, Paola Severgnini, Padelis P. Papadopoulos, Roberto Maiolino, Chiara Feruglio, Ezequiel Treister, George C. Privon, Zhi-yu Zhang, Roberto Della Ceca, Fabrizio Fiore, Kevin Schawinski, and Jeff Wagg

2018 The Astrophysical Journal 863 143.

Provider: AAS Journals

Caption: Figure 2.

Comparison between the CO(2–1) blue and red wing emissions in NGC 6240. For visualization purposes, only positive contours starting from 5σ are shown, with 1σ = 0.33 mJy beam⁻¹ for the blue wing (blue contours) and 1σ = 0.3 mJy beam⁻¹ for the red wing (red contours). The corresponding interferometric maps including negative contours are displayed in Appendix A (Figure 7).

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