MUSE data regarding NGC 3132 were used and analysed through SATELLITE in order to obtain 2D maps of the physico-chemical parameters of the nebula. Furthermore, our results were compared with a 3D photoionisation model built with MOCASSIN with the aim to constrain its parameters. Lastly, we utilized JWST and Spitzer IR data and examined their radial distribution.
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Bouvis et al. (2023) studied this question.
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