The low mas end of the young cluster IC2391

Details The low mas end of the young cluster IC2391 The low mas end of the young cluster IC2391

2002-09-04

arxiv.org/abs/astro-ph/0209065v1

Astronomy and Astrophysics

Astrophysics

To appear in IAU Symp. 211 on "Brown Dwarfs" ed. E. Martin

Scientific paper

By collecting optical and infrared photometry, as well as medium resolution
spectroscopy, we have discovered a sample of low mass stars and brwon dwarfs in
the young cluster IC2391. Using the lithium depletion boundary near the
substellar limit, we have estimated the age of the cluster as ~50 Myr. We have
also estudied the H(alpha) emission in this sample.

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