Figure 2 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 2.

Time evolution of the fiducial run (a = 0.9375); t/t_g = 3000 (top) and 9000 (bottom), respectively. A color-filled contour shows the magnetic energy per unit particle b²/ρ, which is measured in the fluid frame. The BH, the ergosphere (“not hatched”), and two outermost streamlines (genuine parabolic/parabolic), which are anchored to the event horizon, are displayed in the same manner as in Figure 1.

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