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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Ultra-short-period planet formation around late M dwarfs occurs only in fixed close-in or inward-evolving inner disk edge scenarios, as planets follow the edge movement in simulations.
citing papers explorer
-
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.
-
The role of inner disk edges in shaping ultra-short-period planet systems around late M dwarfs
Ultra-short-period planet formation around late M dwarfs occurs only in fixed close-in or inward-evolving inner disk edge scenarios, as planets follow the edge movement in simulations.