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Parabolic Jets from the Spinning Black Hole in M87

  • Authors: Masanori Nakamura, Keiichi Asada, Kazuhiro Hada, Hung-Yi Pu, Scott Noble, Chihyin Tseng, Kenji Toma, Motoki Kino, Hiroshi Nagai, Kazuya Takahashi, Juan-Carlos Algaba, Monica Orienti, Kazunori Akiyama, Akihiro Doi, Gabriele Giovannini, Marcello Giroletti, Mareki Honma, Shoko Koyama, Rocco Lico, Kotaro Niinuma, and Fumie Tazaki

2018 The Astrophysical Journal 868 146.

  • Provider: AAS Journals

Caption: Figure 23.

Variations of ﹩\dot{M}﹩ (top), Φ (middle), and ϕ (bottom) as a function of time with varying BH spin, corresponding to four different cases in Section 3.2. ϕ ≈ 40–60 (MAD state) is indicated as the gray shaded area in the bottom panel.

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