CO isotopolog line fluxes of viscously evolving disks - Cold CO conversion insufficient to explain observed low fluxes

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Fig. C.1

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As Fig. B.1, but showing the ¹³CO (left) and C¹⁸O (right) J = 2− 1 fluxes for allmodels. We note that the range of the y-axes are the same as for Fig. B.1.

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