c-C3H2 deuteration towards prestellar and starless cores in the Perseus molecular cloud

Open Access

Fig. B.2

Column density of the para-c-C₃H₂ 2_1,1 - 2_0,2 transition of Per317 plotted with a colour gradient for a range of $n_{H_{2}}$ $Mathematical equation: ${n_{{{\rm{H}}_2}}}$$ and T_kin. The contour white lines indicate the excitation temperature of the transition, T_ex, and the red cross marks the $n_{H_{2}}$ $Mathematical equation: ${n_{{{\rm{H}}_2}}}$$ and T_kin values derived in Pezzuto et al. (2021).

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