Fig. 6.
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Observed turbulent energy in the discs (Eq. (9)) vs. maximum possible energy that can be injected in the ISM from SNII (Eq. (8)). We explore the possibility of a thin (0.3 kpc, thin ellipse) and a thick disc (1 kpc, thick ellipse). BRI1335−0417 is shown as open marker due to the uncertainties on the dynamical estimate of the gas mass.
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