Probing the Low-Mass Stellar End of the &eta Chamaeleontis Cluster
We have identified three faint new members of the η Chamaeleontis cluster. Spectral types of the new members are estimated to be ∼M5, based on their TiO band strengths and broadband colors. With an age of 5-8 Myr for the cluster, masses of these new me
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
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