Figure 9 from Parabolic Jets from the Spinning Black Hole in M87

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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 9.

Contours (gray) show poloidal magnetic field lines for four different runs with different BH spins (from left to right: a = 0.5, 0.7, 0.9, and 0.99). The final snapshot (t/t_g = 12,000) is displayed for each run with the whole computational domain r/r_g ≤ 100 and 0 ≤ θ ≤ π. Other components in the panels are identical to those in Figure 8.

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