Including the disk buildup phase in protoplanetary disk models produces stronger CO ice enhancement over water in the outer disk but does not yield CO-rich planetesimals without extra mechanisms like pressure traps.
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Dust evolution during protoplanetary disk buildup enhances CO ice relative to water
Including the disk buildup phase in protoplanetary disk models produces stronger CO ice enhancement over water in the outer disk but does not yield CO-rich planetesimals without extra mechanisms like pressure traps.