A uniform reanalysis of 74 resolved millimeter-wave debris belts shows belt dust masses fall with age fastest at small radii, most belts are broad, and vertical thickness shows no age trend.
2018), but moving group age from Zuckerman (2019) -
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REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths
A uniform reanalysis of 74 resolved millimeter-wave debris belts shows belt dust masses fall with age fastest at small radii, most belts are broad, and vertical thickness shows no age trend.