Planet-hosting stars display a bimodal S_phot distribution (peaks at 0.12 and 0.44 rad d^{-1}) absent in controls, with overall enhancement, interpreted as two regimes of magnetic activity coherence.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
No bursty planet-induced radio emission detected from five inactive M dwarfs; upper limits constrain GJ 367 b magnetosphere to <0.8 G under assumed stellar wind conditions.
citing papers explorer
-
Bimodality in Rotational Modulation of Planet-Hosting Stars
Planet-hosting stars display a bimodal S_phot distribution (peaks at 0.12 and 0.44 rad d^{-1}) absent in controls, with overall enhancement, interpreted as two regimes of magnetic activity coherence.
-
Upper Limits on Planet-Induced GHz Radio Emission from Inactive M Dwarfs
No bursty planet-induced radio emission detected from five inactive M dwarfs; upper limits constrain GJ 367 b magnetosphere to <0.8 G under assumed stellar wind conditions.