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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 15.

Comparison of ALMA CO(J = 1–0) integrated intensity (red solid contours) with multiwavelength observations (gray scale). The S-shaped nuclear jet observed with MeerKAT at 1.4 GHz is indicated by blue solid contours in all panels. The filled ellipses at the bottom left of each panel represent the restoring beams for the CO (red) and jet (blue) observations, both outlined with black edges. The gray-scale images are the (a) Chandra X-ray map, (b) MUSE Hα + [N II] map, (c) MeerKAT H I map, (d) HST extinction map, (e) stellar-subtracted Spitzer 8.0 μm map, and (f) stellar-subtracted Spitzer 24 μm map.

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