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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UNVERDICTED 2representative citing papers
Ultra-short-period planet formation around late M dwarfs occurs only in fixed close-in or inward-evolving inner disk edge scenarios, as planets follow the edge movement in simulations.
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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The role of inner disk edges in shaping ultra-short-period planet systems around late M dwarfs
Ultra-short-period planet formation around late M dwarfs occurs only in fixed close-in or inward-evolving inner disk edge scenarios, as planets follow the edge movement in simulations.