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The Low Mass End of the Young Cluster IC2391
Published online by Cambridge University Press: 26 May 2016
Abstract
By collecting optical and infrared photometry, as well as medium resolution spectroscopy, we have discovered a sample of low mass stars and brown 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 studied the Hα emission in this sample.
- Type
- Part 4. Observations of Young Brown Dwarfs (age ≃ 50–200 Myr)
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- Copyright © Astronomical Society of the Pacific 2001
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