Secular perturbations from an inner planet create sharp, marching peaks and caustic discontinuities in a debris disk's azimuthally-averaged surface density, with radial locations following a predictable power-law pattern.
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Reports 23.5% ±2.0% stellar multiplicity rate and 28.8% ±2.1% companion rate for M dwarfs in a 15 pc volume-limited sample from speckle imaging plus literature, with separation peaks at 198 au for planet hosts vs 5.57 au otherwise.
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Debris Disc Substructures Induced by Secular Planetary Perturbations
Secular perturbations from an inner planet create sharp, marching peaks and caustic discontinuities in a debris disk's azimuthally-averaged surface density, with radial locations following a predictable power-law pattern.
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The POKEMON Speckle Survey of Nearby M Dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs within 15 pc
Reports 23.5% ±2.0% stellar multiplicity rate and 28.8% ±2.1% companion rate for M dwarfs in a 15 pc volume-limited sample from speckle imaging plus literature, with separation peaks at 198 au for planet hosts vs 5.57 au otherwise.