Figure 14 from Parabolic Jets from the Spinning Black Hole in M87

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 14.

Similar to Figure 9, but the magnified view is shown for displaying the poloidal magnetic field line around the BH with the computational domain 0 ≤ R/r_g ≤ 20 and −15 ≤ z/r_g ≤ 25. The jet stagnation surface: ﹩{u}^{r}=0﹩ is drawn with navy solid lines on each panel (from upper left to lower right: different BH spins of a = 0.5, 0.7, 0.9, and 0.99, respectively). Orange solid lines in each panel show b²/ρ = 2, 5, 10, and 20, respectively (both at z ≶ 0).

Other Images in This Article

Copyright and Terms & Conditions