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Fig. 11.

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vrms maps centered on Nucleus 2. Left panel: observed MUSE map; in the middle is the best-fit model, and on the right is the same model but without a black hole. The white circle marks the SOI of 0.08″. The typical errors on the vrms values in the MUSE map are 4 km s−1, and thus while the observational scatter appears large it is consistent with the best-fit model in the center with a reduced χ2 of 1.6. We also note the small velocity scale of the colorer, which covers only 18 km s−1 to give sufficient contrast in displaying the models.

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