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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4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 4representative citing papers
A first-principles Bessel gravity kernel resolves the decade-long non-convergence of 2D gravitational-instability simulations and shows that standard Plummer softening overestimates formed fragment masses by a factor of 2–3.
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.
PS16dtm is the tidal disruption of a 0.3 solar-mass star on a circular counter-rotating orbit inside the accretion disk of an NLS1 galaxy, hidden by a gaseous envelope from the observer's view.
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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Self-gravity in thin protoplanetary discs: 2. Numerical convergence solved and revealing the overestimation in mass of formed planets with softening
A first-principles Bessel gravity kernel resolves the decade-long non-convergence of 2D gravitational-instability simulations and shows that standard Plummer softening overestimates formed fragment masses by a factor of 2–3.
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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.
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Tidal disruption of a low-mass star in an active galactic nucleus as the origin of the PS16dtm outburst
PS16dtm is the tidal disruption of a 0.3 solar-mass star on a circular counter-rotating orbit inside the accretion disk of an NLS1 galaxy, hidden by a gaseous envelope from the observer's view.