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Fig. 13


Vertical (top panels) and radial (bottom panels) density profiles (solid lines) during the merger simulations with intervals of 1 Gyr for the FNX-like system: fully collissionless (left), with fgas = 0.3 and fgas = 0.5 (middle), and with fgas = 0.5 including the newly formed stars (right). The dotted lines show the maximum likelyhood fitted profiles: isothermal (sech2) and exponential in the top and bottom panels, respectively.

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