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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 2.

Comparison of HST images to their GALFIT models for each galaxy. Left panels: 2D HST/WFPC2 PC (M32, NGC 5102, NGC 5206) or ACS/HRC (NGC 205) images. Middle panels: fractional residual (Data-Model)/Data between the HST imaging and their corresponding two-component GALFIT models. Right panels: fractional residuals from the three-component GALFIT models. The data and model contours are shown at the same levels of flux and radius in black and white repeating from the left to the right panels, respectively. All figures show east to the left and north up.

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