N-body simulations of main-belt asteroidal dust yield fluxes at inner planets that match scaled Grün and Müller models after calibration, with low-eccentricity grains dominating flux and high-eccentricity grains driving the high-velocity impact tail.
year = 1918, month = oct, volume = 31, pages =
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Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.
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Modeling and Analysis of Main-Belt Asteroidal Dust Flux and Velocity Distribution at Inner Planets
N-body simulations of main-belt asteroidal dust yield fluxes at inner planets that match scaled Grün and Müller models after calibration, with low-eccentricity grains dominating flux and high-eccentricity grains driving the high-velocity impact tail.
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Configuration of the $\xi$ Tau system constrained by multi-technique observations
Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.
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A review summarizing dynamical and physical evolution of Solar System comets and exocomets, highlighting large gaps in exocomet physics due to lack of direct probes.