Fig. 7.
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Same as in Fig. 6, but for modeled data. The models are Jeans spherical models with the indicated types of anisotropy parameters. The models were based on the gravitational potential of NGC 1399 derived in Bílek et al. (2019b) and the parameters of the GCS used in that work. The vertical dashed line at 30′ is an eye-guide to facilitate the reading of the variations of the break radius.
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