Fig. 2.

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Abundance ratios of (14N/15N) × (13C/12C) (left) and 14N/15N with DGC (right). The filled black circles are sources with peak Tmb of H13CN 2–1 lower than 4 K, and the orange stars sources with peak Tmb higher than 4 K. The blue lines are linear fitting results. The cyan parabola was obtained by multiplying the linear regression fit of (14N/15N) × (13C/12C) given in Eq. (3) by the 12C/13C ratio (Eq. (2)). The green, dark green, pink, and magenta lines are the models from Colzi et al. (2022).
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