The low mas end of the young cluster IC2391

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dc.creatorNavascues, David Barrado y
dc.creatorStauffer, John R.
dc.date2002-09-04
dc.date.accessioned2026-07-07T02:04:58Z
dc.date.available2026-07-07T02:04:58Z
dc.descriptionBy 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.
dc.descriptionTo appear in IAU Symp. 211 on "Brown Dwarfs" ed. E. Martin
dc.identifierhttps://arxiv.org/abs/astro-ph/0209065
dc.identifierhttp://arxiv.org/abs/astro-ph/0209065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4965
dc.subjectAstrophysics
dc.titleThe low mas end of the young cluster IC2391
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