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Fig. 6

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Chlorine isotopic ratio, [H35Cl]/[H37Cl], as a function of galac-tocentric radius. The ratio is derived using two methods: R1, which is based on derived XCLASS column densities (for both core and outflow components), and R2, using integrated line intensity ratios. R1 results are further divided into emission and absorption components. Grey symbols indicate the 35Cl/37Cl ratio from previous studies of (a) HCl Peng et al. (2010, pentagons), Cernicharo et al. (2010, octagon), Lis et al. (2010, diamond), and, (b) H2Cl+, Neufeld et al. (2015, white-faced octagon). For context, the Solar System value (3.13; Lodders et al. 2009) and Galactic chemical evolution model predictions for varying metallicities (Kobayashi et al. 2011) are shown using horizontal lines.

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