Evolving protoplanetary disks produce solid C/O and N/O ratios near 1 beyond hypervolatile ice lines, with hypervolatile enhancements up to 100 times higher than static disk models due to drift and advection.
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Icy Volatile Enhancements in Evolving Protoplanetary Disks
Evolving protoplanetary disks produce solid C/O and N/O ratios near 1 beyond hypervolatile ice lines, with hypervolatile enhancements up to 100 times higher than static disk models due to drift and advection.