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.
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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.