SO2 and OCS toward high-mass protostars - A comparative study of ice and gas

Open Access

Fig. G.1

FWHM ratios (upper panel) and V_lsr differences (lower panel) with respect to ${C H}_{3}^{18} O H$ $\[\mathrm{CH}_3^{18} \mathrm{OH}\]$ . For sources in which ${C H}_{3}^{18} O H$ $\[\mathrm{CH}_3^{18} \mathrm{OH}\]$ was not detected by van Gelder et al. (2022a), the main CH₃OH isotopolog was used (empty markers). Values for ³⁴SO₂ are shown in darker colors and for O¹³CS in lighter colors.

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