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.
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Simulations of solar analogues in stellar clusters demonstrate that extended debris disks perturbed by stellar encounters form Oort cloud-like structures and interstellar comets, while compact disks produce Kuiper-belt analogues.
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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.
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Implications for the formation of Oort cloud-like structures and interstellar comets in dense environments
Simulations of solar analogues in stellar clusters demonstrate that extended debris disks perturbed by stellar encounters form Oort cloud-like structures and interstellar comets, while compact disks produce Kuiper-belt analogues.