Thermal instability triggers cyclic MRI activity in protoplanetary disks, enabling dust self-accumulation and planetesimal formation near 1 au with enough mass for multiple super-Earths.
P., Dominik, C., & Natta, A
2 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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Thermal instability and rocky planetesimal formation in the inner regions of protoplanetary disks
Thermal instability triggers cyclic MRI activity in protoplanetary disks, enabling dust self-accumulation and planetesimal formation near 1 au with enough mass for multiple super-Earths.
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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.