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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 1.

Three-color composite image of NGC 1316 from the Fornax Deep Survey (E. Iodice et al. 2016, 2017) using g-, r-, and i-band data obtained with the ESO VLT Survey Telescope. The ALMA observations were conducted to resolve the molecular gas properties within the central region of the galaxy. Red contours represent the CO(J = 1−0) emission map obtained with our ALMA observations. The solid black line indicates the FoV of the ALMA CO(J = 1−0) observations.

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