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Insights into Jet-induced Cloud Disruption in NGC 1316: ALMA Reveals Spatially Extended Molecular Gas

Authors: Kana Morokuma-Matsui, Alexander Y. Wagner, Filippo M. Maccagni, Lauranne Lanz, Fumiya Maeda, Jin Koda, Akihiko Hirota, Yutaka Fujita, Kotaro Kohno, Tomoki Morokuma, Tsutomu T. Takeuchi, Kouichiro Nakanishi, Fumi Egusa, Kenji Bekki, Daniel Espada, Bärbel Koribalski, Jing Wang

Kana Morokuma-Matsui et al 2026 The Astrophysical Journal 1007 .

Provider: AAS Journals

Caption: Figure 11.

R₂₁ and R₃₁ maps using the peak intensity maps of each line in Jy units. The black contours indicate the CO(J = 2−1) integrated intensity map, and the red contours outline the S-shaped nuclear jet. Elevated ratios are observed at several locations along the jet; in particular, the region to the west of the galactic center exhibits relatively high values, with R₂₁ ∼ 4 and R₃₁ ∼ 9.

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