Stellar and Substellar Mass Function of the Young Open Cluster Candidates Alessi 5 and β Monocerotis
Although the stellar and substellar populations have been studied in various young and old open clusters, additional studies in clusters in the the age range from 5 to 100 Myr is crucial (e.g. to give more constrains on initial mass function variation with improved statistics). Among the open cluster candidates from recent studies, two clusters are
Boudreault, S. et al.
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2011