Simulations demonstrate that gas-dust interactions produce radial offsets between micron and millimeter dust in gas-bearing debris disks, depending on gas mass, optical depth, and small-grain abundance.
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2026 2verdicts
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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 ALMA survey to Resolve exoKuiper belt Substructures (ARKS) XI: Gas-dust interactions and radial offsets between micron and millimetre-sized grains
Simulations demonstrate that gas-dust interactions produce radial offsets between micron and millimeter dust in gas-bearing debris disks, depending on gas mass, optical depth, and small-grain abundance.
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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.