Identifying nearby, young, late-type stars by means of their circumstellar disks
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Schneider, A
Song, Inseok
Melis, C
Zuckerman, B
Bessell, Michael
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IOP Publishing
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It has recently been shown that a significant fraction of late-type members of nearby, very young associations (age ≲10Myr) display excess emission at mid-IR wavelengths indicative of dusty circumstellar disks. We demonstrate that the detection of mid-I
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Astrophysical Journal, The
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Open Access
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