Identifying nearby, young, late-type stars by means of their circumstellar disks
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
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Schneider_Identifying_nearby,_young,_2012.pdf||695.88 kB||Adobe PDF|
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