The β Pictoris debris disk is on average 1.5 times thicker vertically in the mid-infrared than at millimeter wavelengths, with a relatively constant scale height across radius and warping consistent with secular perturbations from inner giant planets.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Forward modeling of synthetic debris disc images demonstrates that recovered scattering phase functions are biased by observational limits and do not directly reflect intrinsic dust properties.
citing papers explorer
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The multi-wavelength vertical structure of the archetypal $\beta$ Pictoris debris disk
The β Pictoris debris disk is on average 1.5 times thicker vertically in the mid-infrared than at millimeter wavelengths, with a relatively constant scale height across radius and warping consistent with secular perturbations from inner giant planets.
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What you see is not necessarily what you get: Interpreting near-infrared scattering phase functions of debris discs
Forward modeling of synthetic debris disc images demonstrates that recovered scattering phase functions are biased by observational limits and do not directly reflect intrinsic dust properties.