Fig. 8.
Fraction of IGL by mergers (left panel) and fraction of IGL accreted (right panel), as a function of the BGG stellar mass for four groups: NGC 1316, NGC 5018 (Spavone et al. 2018), NGC 1533 (Cattapan et al. 2019), IC 1459 (Iodice et al. 2020). The shaded areas represent the 20th and 80th percentile of the “model disruption” described by Contini et al. (2014).
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