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.
P., Dominik, C., & Natta, A
3 Pith papers cite this work. Polarity classification is still indexing.
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Dust-free inner disk regions around Herbig stars are molecular-rich environments that dominate CO and H2O line emission between 1 and 28 microns and produce detectable SiO overtone lines.
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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Gas chemistry in the dust depleted inner regions of protoplanetary disks. I. Near-IR spectra and overtones
Dust-free inner disk regions around Herbig stars are molecular-rich environments that dominate CO and H2O line emission between 1 and 28 microns and produce detectable SiO overtone lines.
- Thermal instability and rocky planetesimal formation in the inner regions of protoplanetary disks