Fig. 6.
Top panels: surface brightness maps for the H2 [1-0 S(1)] λ21218 Å, Brγ, Paβ and [Fe II] λ12570 Å emission lines in our Gemini-NIFS NIR observations after subtracting the point-like AGN contribution. The red contours correspond to the distribution of 10 GHz radio continuum emission as resolved with our VLA radio interferometric observations. Lower panels: radial velocity and velocity dispersion for the two brightest lines, H2 and Paβ respectively.
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