Coupled disc-chemistry and N-body simulations identify three classes of giant-planet atmospheres whose elemental ratios (N/O*, C/O*, C/N*, S/N*) trace gas-dominated, planetesimal-dominated, or drift-enhanced accretion in time-dependent discs.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
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Planet formation in chemically diverse and evolving discs II. Chemical fingerprints in planetary atmospheres
Coupled disc-chemistry and N-body simulations identify three classes of giant-planet atmospheres whose elemental ratios (N/O*, C/O*, C/N*, S/N*) trace gas-dominated, planetesimal-dominated, or drift-enhanced accretion in time-dependent discs.
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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.