Figure 8 from Nearby Early-type Galactic Nuclei at High Resolution: Dynamical Black Hole and Nuclear Star Cluster Mass Measurements

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Nearby Early-type Galactic Nuclei at High Resolution: Dynamical Black Hole and Nuclear Star Cluster Mass Measurements

Authors: Dieu D. Nguyen, Anil C. Seth, Nadine Neumayer, Sebastian Kamann, Karina T. Voggel, Michele Cappellari, Arianna Picotti, Phuong M. Nguyen, Torsten Böker, Victor Debattista, Nelson Caldwell, Richard McDermid, Nathan Bastian, Christopher C. Ahn, and Renuka Pechetti

2018 The Astrophysical Journal 858 118.

Provider: AAS Journals

Caption: Figure 8.

A 2D data-model comparison of JAMs with and without BHs. The left panels show maps of V_rms data in each galaxy, the middle panels show the best-fit JAM 2D maps, and the right panels show the best-fit models without a BH. These models are the same as those shown in 1D in Figure 7. The white contours show the continuum, and the red arrows show the orientation.

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