Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars

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Melis, Carl
Zuckerman, B.
Rhee, Joseph H.
Song, Inseok
Murphy, S. J.
Bessell, M. S.

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Cambridge University Press

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We develop a means to distinguish between warm dusty circumstellar debris disks produced by steady state collisional evolution of a planetesimal belt or through transient events.

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Formation, Detection, and Characterization of Extrasolar Habitable Planets

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