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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2 Pith papers cite this work. Polarity classification is still indexing.
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Simulations demonstrate that timescale-based decoupling predictions overestimate separations by a factor of ~3, velocity-based criteria are more accurate, and low-viscosity disks produce decreasing accretion that may identify LISA hosts.
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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The Decoupling of Binaries from Their Circumbinary Disks
Simulations demonstrate that timescale-based decoupling predictions overestimate separations by a factor of ~3, velocity-based criteria are more accurate, and low-viscosity disks produce decreasing accretion that may identify LISA hosts.