Figure 22 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 22.

θ cross section at r/r_g = 100 showing the gas pressure (red solid line), the magnetic pressure (blue solid line), and their sum (the total pressure; black dotted line) for two different initial conditions (a = 0.9 is fixed) at the final stage (t/t_g = 12,000); β_p0,min = 50 (left) and β_p0,min = 500 (right). Readers can refer to the top panel of Figure 10 (a = 0.9) for comparison.

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