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Fig. 7

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CH3OH gas-to-ice ratios (Ngas/Nice) towards low-mass protostars in the Coronet cluster in Corona Australis (triangles). The square and the circle symbolise the average ratios for ten sources in Serpens SVS 4 and four sources in Orion B35A, respectively. The green shaded area corresponds to the interval of gas-to-ice ratios observed for the ten sources in the Serpens SVS 4 cluster. The dotted line indicates the average value for four sources from Öberg et al. (2009a). Upper and lower limits are marked as arrows.

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