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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Protoplanetary disc lifetime distributions are mass-dependent, peaking at 3.72 Myr for high-mass stars and 7.20 Myr for low-mass stars when modeled with Weibull fits assuming an initial disc fraction of 0.8.
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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Disc lifetime distribution as a function of the mass of host star
Protoplanetary disc lifetime distributions are mass-dependent, peaking at 3.72 Myr for high-mass stars and 7.20 Myr for low-mass stars when modeled with Weibull fits assuming an initial disc fraction of 0.8.