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Fig. 2.


Integrated Hα, Hβ, [NII] and [OIII] emission lines from the SINFONI/VLT data in the image plane. The zero velocity corresponds to the center of the Hα emission line. The 1000 realizations obtained with the Monte Carlo simulation are shown in blue and the best fit is shown in black. The gray lines show the positions of skylines.

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