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From dust dynamics to grain propertiesAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Richard Booth. In this talk I will focus on the dust properties we can infer from the observation of its dynamics. I will present two examples. A first, extreme case is the AU Mic debris disk, in which substructures are identified, moving faster than the local escape velocity. A second more generic case is the NIR excess attributed to hot dust around ~20% of the field stars. In both cases, I will show the constraints we can derive from the dynamics on grain size, composition, stellar wind or dust production mechanism. This talk is part of the Exoplanet Seminars series. This talk is included in these lists:
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