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Interplanetary dust around main sequence stars: origin, magnitude, and implications for exoplanet habitability searches

Published onMay 31, 2019
Interplanetary dust around main sequence stars: origin, magnitude, and implications for exoplanet habitability searches
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Abstract

The brightness and spatial distribution of warm (~200K) dust structures located within a few AU We motivate and identify here the main instrumental / observational advances required to gain further insights into the origins of exozodiacal dust clouds and better understand their impact on planetary habitability and habitability searches.

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