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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FLAME pipeline derives stellar luminosities, radii, masses and ages for Gaia DR4 using analytical calculations followed by minimization and Bayesian model inference, with tests showing statistical agreement to literature values.
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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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Stellar masses and ages in Gaia Data Release 4 from the Final Luminosity Age Mass Estimator algorithm
FLAME pipeline derives stellar luminosities, radii, masses and ages for Gaia DR4 using analytical calculations followed by minimization and Bayesian model inference, with tests showing statistical agreement to literature values.