Figure 17 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 17.

Distribution of the jet radius R in NGC 6251 as a function of the jet axial distance z (deprojected with M = 6 × 10⁸ M_⊙ and θ_v = 19°) from the SMBH in units of r_g (T16). This is similar to Figure 15; the vertical/horizontal scales and other components, which are shown in this figure, are identical.

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