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Fig. 19

image

Impact of inner disk radius Rin on CO υ = 1 → 0 line emission fluxes and FWHM. The black line shows the computed R(10) line fluxes for the reference model, when varying Rin between 0.07 AU and 100 AU. The blue line shows the R(10) /R(35) line ratio, and the red line shows the computed R(10) line widths.

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