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We have identified a large sample of probable low mass members of the youngopen cluster IC2391 based on optical (VRIZ) and Infrared (JHK$_s$) photometry.Our sample includes 50 probable members and 82 possible members, both very lowmass stars and brown dwarfs. We also provide accurate positions for these starsand brown dwarf candidates derived from red UK Schmidt plates measured usingthe microdensitometer SuperCOSMOS. Assuming an age of 53 Myr, we estimate thatwe have reached a mass of 0.025 M$_\odot$, if the identified objects are indeedmembers of IC2391.Comment: Accepted Ap

Very Low‐Mass Stars and Brown Dwarfs of the Young Open Cluster IC 2391