Burned to ashes : How the thermal decomposition of refractory organics in the inner protoplanetary disc impacts the gas-phase C/O ratio
The largest reservoir of carbon in protoplanetary discs is stored in refractory organics, which thermally decompose into the gas phase at the organics line located well into the interior of the water iceline. Because this region is so close to the host star, it is often assumed that the released gaseous material is rapidly accreted and has little effect on the evolution of the disc composition. Ho
