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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 3.

Cumulative frequency distribution of the velocity dispersion data shown in Figure 2. The median value (13.3 km s−1) is indicated by the solid gray line. The velocity resolution of the data is 5 km s−1, represented by the gray shaded region. While the majority of the distribution lies below 20 km s−1, there are some regions with dispersions exceeding 50 km s−1.

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