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Fig. 2

image

Logarithm of C2H (N = 3 2, J = 7∕25∕2, F = 43 and F = 32) integrated line luminosity of nine Lupus protoplanetary discs vs. the logarithm of 13CO (J = 3– 2) integrated line flux over the continuum total flux density at 890 μm (integrated over a band width of 1 km s−1 for convenience). The solid grey line shows the typical sensitivity obtained at the distance of our lowest detection (Sz129, at 162 pc).

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