New members of the Scorpius-Centaurus complex and ages of its sub-regions
We have spectroscopically identified ∼100 G-, K-, and M-type members of the Scorpius-Centaurus complex. To deduce the age of these young stars we compare their Liλ6708 absorption line strengths against those of stars in the TW Hydrae association and β
|Collections||ANU Research Publications|
|01_Song_New_members_of_the_2012.pdf||277.76 kB||Adobe PDF|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.