Image Details

Choose export citation format:

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 18.

(Left) Evolution of bubble radius R(t) (left axis) and expansion velocity V(t) (right axis) based on Equation (2). The red solid, blue dashed, and green dotted lines represent the lower limit (Lw = 1.6 × 1043 erg s−1, ne = 0.01 cm−3) and cases where Lw/ρ0 is increased by factors of 10 and 100, respectively. Symbols indicate the expected values at a jet age of 3 Myr, as denoted by the vertical line. (Right) Destruction timescales of molecular clouds as a function of cloud radius. The red solid and blue dashed lines represent the timescales for KH instability (tKHI) and cloud ablation (tabl), respectively. The green dotted and purple dotted–dashed lines correspond to classical and saturated thermal conduction timescales. The horizontal black line indicates the jet age of 3 Myr. The intersection of this reference line with each timescale defines the maximum cloud size that can be fully disrupted within the jet’s lifetime.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse