The spectroscopic characteristics of intermediate-aged pre-main-sequence stars: the &eta Chamaeleontis cluster
We present a study of calibrated low-resolution spectra of the 18 known primaries of the ≈9-Myr-old η Chamaeleontis (η Cha) pre-main-sequence (PMS) star cluster. Using synthetic broad-band colours and narrow-band continuum-sensitive, temperature-sensi
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
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