JWST observations at 15 and 25.5 μm reveal a smooth, radially broad debris disk around γ Ophiuchi extending to 250 au, interpreted as a steady-state collisional cascade from a wide planetesimal belt with possible low-eccentricity planetary perturbation.
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3 Pith papers cite this work, alongside 15 external citations. Polarity classification is still indexing.
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Pith papers citing it
15
external citations · OpenAlex
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2026 3representative citing papers
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.
Spectral synthesis confirms β PsA is nearly pole-on (i≈4.75°) with rapid rotation (Ω/Ωcrit≈0.93), gravity darkening, and true luminosity 26.2 L⊙.
citing papers explorer
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A radially broad collisional cascade in the debris disk of $\gamma$ Ophiuchi observed by JWST
JWST observations at 15 and 25.5 μm reveal a smooth, radially broad debris disk around γ Ophiuchi extending to 250 au, interpreted as a steady-state collisional cascade from a wide planetesimal belt with possible low-eccentricity planetary perturbation.
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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 Debris Disk Host $\beta$ Piscis Austrinus is a Rapidly Rotating Star Seen Nearly Pole-On
Spectral synthesis confirms β PsA is nearly pole-on (i≈4.75°) with rapid rotation (Ω/Ωcrit≈0.93), gravity darkening, and true luminosity 26.2 L⊙.